4th quadrant Galactic SNRs (315°<l<360°)
G315.1+2.7
- Right Ascension: 14 24 30
- Declination: −57 50
- Size (/arcmin): 190×150
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Poorly defined shell.
- Optical: Filaments, brighter in NE.
References:
- Duncan et al. 1997, MNRAS, 287, 722. Parkes 64-m at 2.4 GHz (11': S=19±3 Jy).
ADS
- Combi et al. 1998, A&A, 333, 298. Radio survey observations.
ADS
- Stupar et al. 2007, MNRAS, 374, 1441. Optical and various radio observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 20 May 2014
G315.4−2.3
RCW 86, MSH 14−63
- Right Ascension: 14 43 00
- Declination: −62 30
- Size (/arcmin): 42
- Type: S
- Flux density at 1 GHz (/Jy): 49
- Spectral Index: 0.6
Notes: Possibly the remnant of the SN of AD185?
- Radio: Shell, brightest to the SW.
- Optical: Bright, radiative filaments, with some faint Balmer dominated filaments.
- X-ray: Partial shell, with thermal and non-thermal emission.
- Point sources: Several X-ray sources.
- Distance: Optical observations imply 2.3 kpc.
References:
- van den Bergh et al. 1973, ApJS, 26, 19. Optical observations.
ADS
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=86 Jy) and Parkes 64-m at 5 GHz (4': S=18.2 Jy).
ADS
- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.'4) and 5 GHz (4.'4).
ADS
- Winkler 1978, ApJ, 221, 220. X-ray detection.
ADS
- Leibowitz & Danziger 1983, MNRAS, 204, 273. Optical spectra.
ADS
- Pisarski et al. 1984, ApJ, 277, 710. Einstein observations
ADS
- Nugent et al. 1984, ApJ, 284, 612. X-ray spectrum.
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×50'').
ADS
- Long & Blair 1990, ApJ, 358, L13. Balmer dominated optical filaments.
ADS
- Greidanus & Strom 1990, A&A, 240, 385. IRAS observations.
ADS
- Kaastra et al. 1992, A&A, 264, 654. Ginga X-ray spectra.
ADS
- Strom 1994, MNRAS, 268, L5. Historical association
ADS
- Chin & Huang 1994, Nature, 371, 398. Questioning of historical association.
ADS
- Schaefer 1995, AJ, 110, 1793. Questioning of historical association.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×48'': S>22).
ADS
- Rosado et al. 1996, A&A, 315, 243. Optical kinematics.
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Smith et al. 1997, AJ, 114, 2664. Observations of Balmer dominated filaments.
ADS
- Vink et al. 1997, A&A, 328, 628. ASCA spectroscopy.
ADS
- Bocchino et al. 2000, A&A, 360, 671. BeppoSAX observations of N and SW.
ADS
- Bamba et al. 2000, PASJ, 52, 1157. ASCA observations.
ADS
- Dickel et al. 2001, ApJ, 546, 447. ATCA at 1.34 GHz (8''), including polarisation.
ADS
- Ghavamian et al. 2001, ApJ, 547, 995. Optical spectroscopy.
ADS
- Borkowski et al. 2001, ApJ, 550, 334. ASCA observations.
ADS
- Rho et al. 2002, ApJ, 581, 1116. Chandra observations.
ADS
- Gvaramadze & Vikhlinin 2003, A&A, 401, 625. Chandra point source search.
ADS
- Sollerman et al. 2003, A&A, 407, 249. Optical spectroscopy.
ADS
- Kaplan et al. 2004, ApJS, 153, 269. Chandra limits for any compact source.
ADS
- Bamba et al. 2005, ApJ, 621, 793. Chandra observations of rim.
ADS
- Vink et al. 2006, ApJ, 648, L33. Chandra and XMM-Newton observations.
ADS
- Ueno et al. 2007, PASJ, 59, S171. Suzaku observations.
ADS
- Aharonian et al. 2009, ApJ, 692, 1500. HESS observations.
ADS
- Yamaguchi et al. 2011, PASJ, 63, S837. Suzaku observations.
ADS
- Helder et al. 2011, ApJ, 737, 85. XMM-Newton and optical observations.
ADS
- Williams et al. 2011, ApJ, 741, 96. Spitzer observations.
ADS
- Mignani et al. 2012, MNRAS, 425, 2309. X-ray and optical observations of compact X-ray sources.
ADS
- Lemoine-Goumard et al. 2012, A&A, 545, A28. Fermi observations.
ADS
- Helder et al. 2013, MNRAS, 435, 910. Optical proper motion studies.
ADS
- Castro et al. 2013, ApJ, 779, 49. Chandra of NW.
ADS
- Yuan et al. 2014, ApJ, 785, L22. Fermi observations.
ADS
- Tsubone et al. 2014, in EFXU, p72. Suzaku observations.
ADS
- Broersen et al. 2014, MNRAS, 441, 3040. XMM-Newton observations.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 30, 44 and 70 GHz.
ADS
- Ajello et al. 2016, ApJ, 819, 98. Fermi observations, and ATCA HI of surroundings.
ADS
- Yamaguchi et al. 2016, ApJ, 820, L3. Chandra observations of NE.
ADS
- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
ADS
- Tsubone et al. 2017, ApJ, 835, 34. Suzaku observations.
ADS
- Sano et al. 2017, JHEAp, 15, 1. CO and HI observations.
ADS
- Abramowski et al. 2018, A&A, 612, A4. HESS observations.
ADS
Last updated: 15 Apr 2019
G315.4−0.3
- Right Ascension: 14 35 55
- Declination: −60 36
- Size (/arcmin): 24×13
- Type: ?
- Flux density at 1 GHz (/Jy): 8
- Spectral Index: 0.4
- Radio: Irregular non-thermal emission, with HII region superposed in E.
- Optical: Detected.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=15.9 Jy) and Parkes 64-m at 5 GHz (4': S=4.9 Jy).
ADS
- Caswell et al. 1981, MNRAS, 195, 89. FIRST at 1415 MHz (50'': S=6.25 Jy), re-assessment of earlier flux densities.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×49'': S=3.1 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 25 Apr 2014
G315.9−0.0
- Right Ascension: 14 38 25
- Declination: −60 11
- Size (/arcmin): 25×14
- Type: S
- Flux density at 1 GHz (/Jy): 0.8?
- Spectral Index: ?
Notes: Has been called G315.8−0.0.
- Radio: Faint, distorted shell, with elongated trail to pulsar.
- Point sources: Pulsar at end of radio trail.
References:
- Kesteven et al. 1987, AuJPh, 40, 855. MOST at 843 MHz (44''×50'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S=0.9 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m and ATCA OH observations.
ADS
- Camilo et al. 2009, ApJ, 703, L55. Pulsar detection.
ADS
- Ng et al. 2012, ApJ, 746, 105. ATCA at 1.4, 2.5, 5 and 9 GHz, including polarisation, of pulsar trail.
ADS
Last updated: 24 Apr 2014
G316.3−0.0
(MSH 14−57)
- Right Ascension: 14 41 30
- Declination: −60 00
- Size (/arcmin): 29×14
- Type: S
- Flux density at 1 GHz (/Jy): 20?
- Spectral Index: 0.4
- Radio: Distorted shell, with possible `blowout'.
- X-ray: Detected.
- Distance: HI absorption data suggests >7.2 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.'4: S=16.7 Jy).
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×51'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S=20 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 13 May 2017
G317.3−0.2
- Right Ascension: 14 49 40
- Declination: −59 46
- Size (/arcmin): 11
- Type: S
- Flux density at 1 GHz (/Jy): 4.7?
- Spectral Index: ?
- Radio: Incomplete shell.
- Optical: Detected.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S=5.2 Jy).
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 25 Apr 2014
G318.2+0.1
- Right Ascension: 14 54 50
- Declination: −59 04
- Size (/arcmin): 40×35
- Type: S
- Flux density at 1 GHz (/Jy): >3.9?
- Spectral Index: ?
- Radio: Faint shell, with central HII region.
- X-ray: Sources within remnant.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S>4.3).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Bocchino et al. 2001, A&A, 367, 629. BeppoSAX and ROSAT observations.
ADS
- Onako et al. 2016, ApJ, 829, 106. Akari observations.
ADS
Last updated: 13 May 2017
G318.9+0.4
- Right Ascension: 14 58 30
- Declination: −58 29
- Size (/arcmin): 30×14
- Type: C
- Flux density at 1 GHz (/Jy): 4?
- Spectral Index: 0.2?
Notes: May not be a SNR?
- Radio: Complex arcs, with off-centre core.
References:
- Whiteoak 1990, Nature, 347, 157. MOST at 843 MHz (43''×51'').
ADS
- Whiteoak 1993, ApJ, 415, 701. MOST at 843 MHz (43''×51'': S=4.8±0.6 Jy), Parkes 64-m at 4.5 GHz (4.'7: S=3.7±0.2 Jy) and 8.4 GHz (2.'8: S=3.0±0.4 Jy) including polarisation, and ATCA at 1.4 GHz and 4.8 GHz (11''×13'') of core.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S=4.8 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G320.4−1.2
MSH 15−52, RCW 89
- Right Ascension: 15 14 30
- Declination: −59 08
- Size (/arcmin): 35
- Type: C
- Flux density at 1 GHz (/Jy): 60?
- Spectral Index: 0.4
Notes: Has been suggested as the remnant of the SN of AD185?
- Radio: Ragged shell.
- Optical: RCW 89 is the Hα emitting region to the NW.
- X-ray: Partial shell, central nebula and pulsar and `jet'.
- Point sources: Radio and X-ray pulsar, with wind nebula.
- Distance: HI absorption indicates 5.2 kpc.
References:
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.'4) and 5 GHz (4.'4).
ADS
- Dopita et al. 1977, ApJ, 214, 179. Optical spectra.
ADS
- Caswell et al. 1981, MNRAS, 195, 89. FIRST at 1415 MHz (50'').
ADS
- Seward & Harnden 1982, ApJ, 256, L45. X-ray observations of pulsar.
ADS
- Manchester et al. 1982, ApJ, 262, L31. Radio observations of pulsar.
ADS
- Seward et al. 1983, ApJ, 267, 698. X-ray, Optical and IR.
ADS
- van den Bergh & Kamper 1984, ApJ, 280, L51. Optical expansion.
ADS
- Seward et al. 1984, ApJ, 281, 650. X-ray observations of pulsar and nebulosity.
ADS
- Lortet et al. 1987, A&A, 180, 65. Optical observations.
ADS
- Trussoni et al. 1990, A&A, 234, 403. EXOSAT observations.
ADS
- Asaoka & Koyama 1990, PASJ, 42, 625. Ginga X-ray spectrum.
ADS
- Arendt 1991, AJ, 101, 2160. IRAS observations, including compact source.
ADS
- Milne et al. 1993, MNRAS, 264, 853. Parkes 64-m at 4.8 GHz (4.'5: S=37±7 Jy) and 8.4 GHz (3.'0: S=24±4 Jy), including polarisation and review of flux densities.
ADS
- Strom 1994, MNRAS, 268, L5. Historical association.
ADS
- Chin & Huang 1994, Nature, 371, 398. Questioning of historical association.
ADS
- Matz et al. 1994, ApJ, 434, 288. X-ray observations of pulsar.
ADS
- Schaefer 1995, AJ, 110, 1793. Questioning of historical association.
ADS
- Du Plessis et al. 1995, ApJ, 453, 746. Hartesbeesthoek 26-m at 2.3, 5 and 8.5 GHz (S=42, 35.6 and 14.5 Jy).
ADS
- Greiveldinger et al. 1995, ApJ, 454, 855. ROSAT observations.
ADS
- Trussoni et al. 1996, A&A, 306, 581. ROSAT observations.
ADS
- Tamura et al. 1996, PASJ, 48, L33. ASCA observations.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S=62 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Marsden et al. 1997, ApJ, 491, L39. X-ray spectroscopy.
ADS
- Brazier & Becker 1997, MNRAS, 284, 335. ROSAT observations.
ADS
- Gaensler et al. 1999, MNRAS, 305, 724. ATCA at 1.4 GHz (21''×24''), plus HI observations, and 5.3 GHz (10''×15'').
ADS
- Sako et al. 2000, ApJ, 537, 422. Possible γ-ray detection of pulsar.
ADS
- Mineo et al. 2001, A&A, 380, 695. BeppoSAX observations.
ADS
- Gaensler et al. 2002, ApJ, 569, 878. Chandra observations of pulsar and nebula.
ADS
- Dubner et al. 2002, AJ, 123, 337. ATCA at 1.4 GHz (2.'7×4.'0), plus HI observations.
ADS
- Aharonian et al. 2005, A&A, 435, L17. HESS detection.
ADS
- Yatsu et al. 2005, ApJ, 631, 312. Chandra observations of pulsar and jet.
ADS
- DeLaney et al. 2006, ApJ, 640, 929. Chandra and ROSAT multi-epoch observations of pulsar wind nebula.
ADS
- Kaplan & Moon 2006, ApJ, 644, 1056. Possible IR detection of pulsar.
ADS
- Forot et al. 2006, ApJ, 651, L45. X-ray observations of pulsar and nebula.
ADS
- Nakamori et al. 2008, ApJ, 677, 297. γ-ray observations.
ADS
- Yatsu et al. 2009, PASJ, 61, 129. Chandra observations of pulsar wind nebula.
ADS
- Koo et al. 2011, ApJ, 732, 6. Akari and Spitzer observations.
ADS
- An et al. 2014, ApJ, 793, 90. NuSTAR observations of PWN.
ADS
- Abdalla et al. 2018, A&A, 612, A1. HESS observations.
ADS
Last updated: 15 Apr 2019
G320.6−1.6
- Right Ascension: 15 17 50
- Declination: −59 16
- Size (/arcmin): 60×30
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Faint shell, overlapping G320.4−1.2 in W.
- Optical: Detected.
References:
- Milne et al. 1993, MNRAS, 264, 853. Parkes 64-m at 4.8 GHz (4.'5) and 8.4 GHz (3.'0), including polarisation.
ADS
- Duncan et al. 1995, MNRAS, 277, 36. Parkes 64-m at 2.4-GHz (10.'4).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×50'': S>9.3).
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 25 Apr 2014
G321.9−1.1
- Right Ascension: 15 23 45
- Declination: −58 13
- Size (/arcmin): 28
- Type: S
- Flux density at 1 GHz (/Jy): >3.4?
- Spectral Index: ?
- Radio: Faint shell.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×51'': S>3.8).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 7 Jan 2004
G321.9−0.3
- Right Ascension: 15 20 40
- Declination: −57 34
- Size (/arcmin): 31×23
- Type: S
- Flux density at 1 GHz (/Jy): 13
- Spectral Index: 0.3
- Radio: Shell brighter to the W, with Cir X-1 to N.
- Point sources: Pulsar near E edge.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=18.3 Jy) and Parkes 64-m at 5 GHz (4': S=7.8 Jy).
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×52'').
ADS
- Stewart et al. 1993, MNRAS, 261, 593. ATCA at 1.5 GHz (21'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×51'': S>8.3).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Mignani et al. 2002, A&A, 386, 487. HST proper motion study of Cir X-1.
ADS
- Tudose et al. 2006, MNRAS, 372, 417. MOST at 843 MHz.
ADS
- Pletsch et al. 2013, ApJ, 779, L11. Pulsar detection.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 8 Jun 2019
G322.1+0.0
- Right Ascension: 15 20 49
- Declination: −57 10
- Size (/arcmin): 8×4.5?
- Type: S?
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Circular shell, with extension to S.
- X-ray: Diffuse emission.
- Point sources: Cir X-1 HMXB at centre.
References:
- Heinz et al. 2013, ApJ, 779, 171. Chandra observations and ATCA at 1.1–3.1 GHz (4.''0×4.''9).
ADS
Last updated: 30 Apr 2014
G322.5−0.1
- Right Ascension: 15 23 23
- Declination: −57 06
- Size (/arcmin): 15
- Type: C
- Flux density at 1 GHz (/Jy): 1.5
- Spectral Index: 0.4
- Radio: Shell with central extended source.
- Point sources: PN Pe 2-8 within boundary.
References:
- Whiteoak 1992, MNRAS, 256, 121. MOST at 843 MHz (43''×51'': S=2.0±0.3 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×51'': S=1.7 Jy), plus Parkes 64-m at 4.5 GHz (=0.89±0.13).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G323.5+0.1
- Right Ascension: 15 28 42
- Declination: −56 21
- Size (/arcmin): 13
- Type: S
- Flux density at 1 GHz (/Jy): 3?
- Spectral Index: 0.4?
- Radio: Distorted shell, confused with thermal emission.
- Point sources: Compact, probably thermal source near centre.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=4.2 Jy) and Parkes 64-m at 5 GHz (4': S=1.5 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×52'': S=4.2 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
Last updated: 16 Mar 2009
G323.7−1.0
- Right Ascension: 15 34 30
- Declination: −57 12
- Size (/arcmin): 51×38
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Faint shell.
- X-ray: Faint diffuse emission.
- Distance: CO and HI observations suggest 3.5 kpc.
References:
- Green et al. 2014, PASA, 31, 42. MGPS observations at 843 MHz (43''×51'').
ADS
- Araya et al. 2017, ApJ, 843, 12. Fermi observations.
ADS
- Abdalla et al. 2018, A&A, 612, A8. HESS observations.
ADS
- Maxted et al. 2018, MNRAS, 480, 134. CO and HI observations.
ADS
- Saji et al. 2018, PASJ, 70, 23. Suzaku observations.
ADS
Last updated: 16 Apr 2019
G326.3−1.8
MSH 15−56
- Right Ascension: 15 53 00
- Declination: −56 10
- Size (/arcmin): 38
- Type: C
- Flux density at 1 GHz (/Jy): 145
- Spectral Index: varies
Notes: Has been called G326.2−1.7.
- Radio: Shell, with elongated, flat-spectrum core.
- Optical: Emission around the shell.
- X-ray: Shell, with central extended emission.
- Point sources: Compact X-ray source.
References:
- Clark et al. 1975, AuJPA, 37, 75. Molonglo at 408 MHz (3': S=180 Jy).
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Milne et al. 1979, MNRAS, 188, 437. FIRST at 1415 MHz (0.'8: S>95) and Parkes 64-m at 14.7 GHz (2.'2: S=69±8 Jy).
ADS
- van den Bergh 1979, ApJ, 227, 497. Optical observations.
ADS
- Zealey et al. 1979, A&AS, 38, 39. Optical observations.
ADS
- Dennefeld 1980, PASP, 92, 603. Optical spectra.
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×53'').
ADS
- Milne et al. 1989, PASA, 8, 187. MOST at 843 MHz (43''×52'': S=153±40 Jy), and Parkes 64-m at 8.4 GHz (3': S=68±5 Jy), including polarisation.
ADS
- Seward 1990, ApJS, 73, 781. Einstein observations.
ADS
- Kassim et al. 1993, ApJ, 419, 733. ROSAT image.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×52'': S>130).
ADS
- Rosado et al. 1996, A&A, 315, 243. Optical kinematics.
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Dickel et al. 2000, ApJ, 543, 840. ATCA at 1.34 GHz (6.''4×8.''5: S>60 Jy), 4.80 GHz (3.''8: S=25 Jy for core only) and 8.64 GHz (3.''2: S=15 Jy for core only).
ADS
- Temim et al. 2013, ApJ, 768, 61. XMM-Newton and Chandra observations.
ADS
- Yatsu et al. 2013, ApJ, 773, 25. XMM-Newton and Chandra observations.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 5 frequencies between 30 and 143 GHz.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Temim et al. 2017, ApJ, 851, 128. Chandra proper motion study of central source.
ADS
- Devin et al. 2018, A&A, 617, A5. Fermi observations.
ADS
Last updated: 9 Apr 2019
G327.1−1.1
- Right Ascension: 15 54 25
- Declination: −55 09
- Size (/arcmin): 18
- Type: C
- Flux density at 1 GHz (/Jy): 7?
- Spectral Index: ?
- Radio: Shell, with off-centre core.
- X-ray: Diffuse, with core.
References:
- Milne & Dickel 1974, AuJPh, 27, 549. Parkes 64-m at 2.7 GHz (8.'4: S=10±15% Jy).
ADS
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=10.6 Jy) and Parkes 64-m at 5 GHz (4': S=4.3 Jy).
ADS
- Lamb & Markert 1981, ApJ, 244, 94. Einstein observations.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×52'': S=7.6 Jy).
ADS
- Seward et al. 1996, ApJ, 471, 887. ROSAT observations.
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Sun et al. 1999, ApJ, 511, 274. ASCA and ROSAT observations.
ADS
- Bocchino & Bandiera 2003, A&A, 398, 195. BeppoSAX observations.
ADS
- Temim et al. 2009, ApJ, 691, 895. Chandra and XMM-Newton observations.
ADS
- Temim et al. 2015, ApJ, 808, 100. Chandra observations.
ADS
- Ma et al. 2016, ApJ, 820, 100. ATCA at 1.4 (19''×23''), 2.3 (11''×16''), 4.8 (13''×15'') and 8.6 GHz (8''×10'') of core, including polarisation.
ADS
- Abdalla et al. 2018, A&A, 612, A1. HESS observations.
ADS
Last updated: 23 Apr 2019
G327.2−0.1
- Right Ascension: 15 50 55
- Declination: −54 18
- Size (/arcmin): 5
- Type: S
- Flux density at 1 GHz (/Jy): 0.4
- Spectral Index: ?
Notes: Has been called G327.24−0.13.
- Radio: Shell, possibly with central emission.
- Point sources: Central pulsar (magnetar).
References:
- Camilo et al. 2007, ApJ, 666, L93. Pulsar observations.
ADS
- Gelfand & Gaensler 2007, ApJ, 667, 1111. Chandra and XMM-Newton observations of magnetar, and 843 GHz (43''×53'': S=0.5±0.1 Jy) and SGPS at 1.4 GHz (S=0.3±0.1 Jy).
ADS
Last updated: 20 Apr 2019
G327.4+0.4
Kes 27
- Right Ascension: 15 48 20
- Declination: −53 49
- Size (/arcmin): 21
- Type: S
- Flux density at 1 GHz (/Jy): 30?
- Spectral Index: 0.6
Notes: Has been called G327.3+0.4 and G327.3+0.5.
- Radio: Incomplete, multi-arc shell, brightest to the SE.
- X-ray: Diffuse, brighter in E.
- Distance: HI absorption indicates 4.3 to 5.4 kpc.
References:
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=58 Jy) and Parkes 64-m at 5 GHz (4': S=12.4 Jy).
ADS
- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.'4) and 5 GHz (4.'4).
ADS
- Lamb & Markert 1981, ApJ, 244, 94. Einstein observations.
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×55'').
ADS
- Milne et al. 1989, PASA, 8, 187. MOST at 843 MHz (43''×53'': S=32.2±6 Jy), and Parkes 64-m at 8.4 GHz (3': S=9.4±0.8 Jy), including polarisation.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×53'': S=25 Jy).
ADS
- Seward et al. 1996, ApJ, 471, 887. ROSAT observations.
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m and ATCA OH observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
- Enoguchi et al. 2002, PASJ, 54, 229. ASCA observations.
ADS
- Kawasaki et al. 2005, ApJ, 631, 935. ASCA observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- Chen et al. 2008, ApJ, 676, 1040. Chandra observations.
ADS
- Minami et al. 2014, in EFXU, p48. Suzaku observations.
ADS
- Xing et al. 2015, ApJ, 805, 19. Fermi observations.
ADS
Last updated: 12 Jun 2017
G327.4+1.0
- Right Ascension: 15 46 48
- Declination: −53 20
- Size (/arcmin): 14
- Type: S
- Flux density at 1 GHz (/Jy): 1.9?
- Spectral Index: ?
- Radio: Asymmetric shell.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×54'': S=2.1 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
Last updated: 10 Oct 2001
G327.6+14.6
SN1006, PKS 1459−41
- Right Ascension: 15 02 50
- Declination: −41 56
- Size (/arcmin): 30
- Type: S
- Flux density at 1 GHz (/Jy): 19
- Spectral Index: 0.6
Notes: This is the remnant of the SN of AD1006.
- Radio: Shell, with two bright arcs.
- Optical: Filaments to the NW, with broad Hα component.
- X-ray: Thermal shell, with non-thermal limb-brightened arcs.
- Point sources: The background Schweizer–Middleditch star is near the middle of the remnant.
- Distance: Optical spectra and proper motion indicate 1.85 kpc.
References:
- van den Bergh 1976, ApJ, 208, L17. Optical observations.
ADS
- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.'4) and 5 GHz (4.'4).
ADS
- Schweizer & Middleditch 1980, ApJ, 241, 1039. Possible stellar remnant.
ADS
- Caswell et al. 1983, MNRAS, 204, 921. FIRST at 1415 MHz (77'').
ADS
- Reynolds & Gilmore 1986, AJ, 92, 1138. VLA at 1.37 and 1.67 GHz (16''×20'').
ADS
- Kirshner et al. 1987, ApJ, 315, L135. Broad Hα optical component.
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×66'').
ADS
- Fesen et al. 1988, ApJ, 327, 164. UV absorption spectra of the Schweizer–Middleditch star.
ADS
- Roger et al. 1988, ApJ, 332, 940. MOST at 843 MHz (44''×66'': S=17.5±1.5 Jy).
ADS
- Long et al. 1988, ApJ, 333, 749. Optical proper motion for distance.
ADS
- Wu et al. 1993, ApJ, 416, 247. UV spectra.
ADS
- Reynolds & Gilmore 1993, AJ, 106, 272. VLA at 1.37 and 1.67 GHz (24''), including polarisation.
ADS
- Moffett et al. 1993, AJ, 106, 1566. VLA at 1.37 and 1.67 GHz (10''×14''), for proper motion studies.
ADS
- Ozaki et al. 1994, PASJ, 46, 367. X-ray observations.
ADS
- Raymond et al. 1995, ApJ, 454, L31. Far UV spectroscopy.
ADS
- Koyama et al. 1995, Nature, 378, 255. ASCA observations.
ADS
- Willingale et al. 1996, MNRAS, 278, 749. ROSAT observations.
ADS
- Blair et al. 1996, ApJ, 468, 871. Optical absorption studies.
ADS
- Laming et al. 1996, ApJ, 472, 267. Modelling of optical spectra, including distance.
ADS
- Wu et al. 1997, ApJ, 477, L53. Far UV absorption spectra of the Schweizer–Middleditch star.
ADS
- Winkler & Long 1997, ApJ, 486, L137. UV absorption spectra of background quasar.
ADS
- Winkler & Long 1997, ApJ, 491, 829. ROSAT and optical images.
ADS
- Vink et al. 2000, A&A, 354, 931. X-ray spectroscopy.
ADS
- Burleigh et al. 2000, A&A, 356, 585. Optical spectroscopy of the Schweizer–Middleditch star.
ADS
- Allen et al. 2001, ApJ, 558, 739. ASCA, ROSAT and other X-ray observations.
ADS
- Dubner et al. 2002, A&A, 387, 1047. ATCA at 1.4 GHz (3.'0×4.'7) for HI, plus CO observations.
ADS
- Ghavamian et al. 2002, ApJ, 572, 888. Optical of filaments in NW.
ADS
- Sollerman et al. 2003, A&A, 407, 249. Optical spectroscopy.
ADS
- Winkler et al. 2003, ApJ, 585, 324. Optical proper motion studies.
ADS
- Vink et al. 2003, ApJ, 587, L31. XMM-Newton observations.
ADS
- Bamba et al. 2003, ApJ, 589, 827. Chandra observations of NE.
ADS
- Winkler et al. 2005, ApJ, 624, 189. HST absorption towards background sources.
ADS
- Kalemci et al. 2006, ApJ, 644, 274. INTEGRAL observations.
ADS
- Acero et al. 2007, A&A, 475, 883. XMM-Newton observations.
ADS
- Raymond et al. 2007, ApJ, 659, 1257. HST Hα observations.
ADS
- Hamilton et al. 2007, MNRAS, 381, 771. UV spectroscopy of the Schweizer–Middleditch star.
ADS
- Bamba et al. 2008, AdSpR, 41, 411. Suzaku observations.
ADS
- Cassam-Chenaï et al. 2008, ApJ, 680, 1180. ATCA and VLA at 1.5 GHz (6''×9'') plus Chandra observations.
ADS
- Yamaguchi et al. 2008, PASJ, 60, S141. Suzaku observations.
ADS
- Dyer et al. 2009, AJ, 137, 2956. GBT and VLA observations at 1.4 GHz.
ADS
- Winkler et al. 2011, ApJ, 742, 80. Multi-epoch UV spectroscopy of the Schweizer–Middleditch star.
ADS
- Miceli et al. 2013, A&A, 550, A80. XMM-Newton observations.
ADS
- Broersen et al. 2013, A&A, 552, A9. XMM-Newton observations of NW knot.
ADS
- Katsuda et al. 2013, ApJ, 763, 85. Chandra proper motion study of NW.
ADS
- Winkler et al. 2013, ApJ, 764, 156. Spitzer observations.
ADS
- Uchida et al. 2013, ApJ, 771, 56. Suzaku observations.
ADS
- Reynoso et al. 2013, AJ, 145, 104. VLA and ATCA at 1.4 GHz (10''), including polarisation.
ADS
- Nikolić et al. 2013, Science, 340, 45. Optical spectroscopy.
ADS
- Winkler et al. 2014, ApJ, 781, 65. Chandra observations and Hα spectroscopy.
ADS
- Miceli et al. 2014, ApJ, 782, L33. XMM-Newton observations of SW.
ADS
- Acero et al. 2015, A&A, 580, A74. Fermi limit.
ADS
- Sparls et al. 2015, ApJ, 815, L9. Polarised optical line observations.
ADS
- Li et al. 2015, MNRAS, 453, 3953. XMM-Newton observations.
ADS
- Arnaud et al. 2016, A&A, 586, A134. Planck flux densities at 4 frequencies between 30 and 100 GHz.
ADS
- Xing et al. 2016, ApJ, 823, 44. Fermi observations.
ADS
- Li et al. 2016, MNRAS, 462, 158. XMM-Newton observations.
ADS
- Raymond et al. 2017, ApJ, 851, 12. UV and optical spectra, for proper motions and distance.
ADS
- Condon et al. 2017, ApJ, 851, 100. Fermi observations.
ADS
- Kerzendorf et al. 2018, MNRAS, 479, 192. Optical search for progenitor companion.
ADS
- Li et al. 2018, ApJ, 864, 85. NuSTAR observations of NE and SW limbs.
ADS
Last updated: 9 Apr 2019
G328.4+0.2
(MSH 15−57)
- Right Ascension: 15 55 30
- Declination: −53 17
- Size (/arcmin): 5
- Type: F
- Flux density at 1 GHz (/Jy): 15
- Spectral Index: 0.0
- Radio: Amorphous emission, with central bar.
- X-ray: Detected at high energies.
- Distance: HI absorption indicates >17.4 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Caswell et al. 1980, MNRAS, 190, 881. FIRST at 1415 MHz (50'').
ADS
- Wilson 1986, ApJ, 302, 718. Lack of detection with Einstein.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×54'': S=15 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Gaensler et al. 2000, ApJ, 542, 380. ATCA at 1.4 GHz (16.''5×19.''5: S=14.3±0.1 Jy) and 4.5 GHz (1.''5×2.''0: S=12.5±0.2 Jy).
ADS
- Hughes et al. 2000, ApJ, 542, 386. ASCA observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
- Johnston et al. 2004, MNRAS, 348, L19. ATCA at 19 GHz (6.''1×7.''7), including polarisation.
ADS
- Gelfand et al. 2007, ApJ, 663, 468. ATCA at 1.4 GHz (5.''8×7.''0: S=13.8±0.4 Jy), plus XMM-Newton observations.
ADS
Last updated: 27 Mar 2009
G329.7+0.4
- Right Ascension: 16 01 20
- Declination: −52 18
- Size (/arcmin): 40×33
- Type: S
- Flux density at 1 GHz (/Jy): >34?
- Spectral Index: ?
- Radio: Diffuse shell, in complex region.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×53'': S>38).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
Last updated: 16 Mar 2009
G330.0+15.0
Lupus Loop
- Right Ascension: 15 10 00
- Declination: −40 00
- Size (/arcmin): 180?
- Type: S
- Flux density at 1 GHz (/Jy): 350?
- Spectral Index: 0.5?
- Radio: Low surface brightness loop with HI shell.
- X-ray: Detected, with central source.
- Point sources: Central, possibly pulsating, X-ray source.
References:
- Milne 1971, AuJPh, 24, 757. Parkes 64-m at 408 MHz (48'), 635 MHz (31') and 1410 MHz (15').
ADS
- Milne & Dickel 1974, AuJPh, 27, 549. Parkes 64-m at 2.7 GHz (8.'4: S=120±30% Jy).
ADS
- Toor 1980, A&A, 85, 184. X-ray image and spectrum.
ADS
- Colomb & Dubner 1982, A&A, 112, 141. Argentine 30-m dish at 1.42 GHz (30'), HI observations.
ADS
- Leahy et al. 1991, ApJ, 374, 218. HEAO-1 X-ray spectra.
ADS
- Ozaki et al. 1994, PASJ, 46, 367. X-ray observations.
ADS
- Kaplan et al. 2006, ApJS, 163, 344. X-ray upper limit on compact sources.
ADS
- Shinn et al. 2006, ApJ, 644, L189. Far UV observations.
ADS
Last updated: 30 May 2014
G330.2+1.0
- Right Ascension: 16 01 06
- Declination: −51 34
- Size (/arcmin): 11
- Type: S?
- Flux density at 1 GHz (/Jy): 5?
- Spectral Index: 0.3
- Radio: Clumpy non-thermal emission, possibly a distorted shell.
- X-ray: Shell.
- Point sources: Central compact X-ray source.
- Distance: HI absorption indicates >4.9 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=8.6 Jy) and Parkes 64-m at 5 GHz (4': S=4.0 Jy).
ADS
- Caswell et al. 1983, MNRAS, 204, 915. FIRST at 1415 MHz (47''×52''), and MOST at 843 MHz (43''×55'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×55'': S=4.7 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
- Torii et al. 2006, PASJ, 58, L11. ASCA detection.
ADS
- Park et al. 2009, ApJ, 695, 431. XMM-Newton and Chandra observations.
ADS
- Abramowski et al. 2014, MNRAS, 441, 790. HESS upper limit.
ADS
- Doroshenko et al. 2018, A&A, 619, A26. XMM-Newton observations of central source.
ADS
- Williams et al. 2018, ApJ, 855, 118. XMM-Newton observations.
ADS
- Borkowski et al. 2018, ApJ, 868, L21. Chandra observations for expansion study.
ADS
Last updated: 9 Apr 2019
G332.0+0.2
- Right Ascension: 16 13 17
- Declination: −50 53
- Size (/arcmin): 12
- Type: S
- Flux density at 1 GHz (/Jy): 8?
- Spectral Index: 0.5
- Radio: Incomplete shell.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×57'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×55'': S=8.9 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- McClure-Griffiths et al. 2001, ApJ, 551, 394. ATCA and Parkes 64-m at 1.4 GHz (1.'8×2.'0), plus HI.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 13 May 2017
G332.4−0.4
RCW 103
- Right Ascension: 16 17 33
- Declination: −51 02
- Size (/arcmin): 10
- Type: S
- Flux density at 1 GHz (/Jy): 28
- Spectral Index: 0.5
- Radio: Shell, brightest to the S.
- Optical: Filaments correspond well to the radio shell, brightest in SE.
- X-ray: Brightest to NW, with point source near centre.
- Point sources: Central, variable X-ray source, and nearby pulsar.
- Distance: HI absorption indicates 3.1 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Tuohy & Garmire 1980, ApJ, 239, L107. Einstein detection of X-ray point source.
ADS
- Caswell et al. 1980, MNRAS, 190, 881. FIRST at 1415 MHz (50'').
ADS
- Lamb & Markert 1981, ApJ, 244, 94. Einstein observations.
ADS
- Ruiz 1983, AJ, 88, 1210. Optical spectra.
ADS
- Tuohy et al. 1983, ApJ, 268, 778. X-ray observations.
ADS
- Leibowitz & Danziger 1983, MNRAS, 204, 273. Optical spectra.
ADS
- Nugent et al. 1984, ApJ, 284, 612. X-ray spectrum (and Einstein image from Tuohy, private communication).
ADS
- Meaburn & Allen 1986, MNRAS, 222, 593. Optical spectra.
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×57'').
ADS
- Oliva et al. 1990, A&A, 240, 453. IR spectroscopy.
ADS
- Dickel et al. 1996, AJ, 111, 340. ATCA at 1.36 (8'') and 2.37 GHz (4.''5''), including polarisation.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×55'': S=34 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
ADS
- Gotthelf et al. 1997, ApJ, 487, L175. ASCA observations of compact X-ray source.
ADS
- Carter et al. 1997, PASP, 109, 990. Optical expansion.
ADS
- Torii et al. 1998, ApJ, 494, L207. ASCA detection of nearby pulsar.
ADS
- Kaspi et al. 1998, ApJ, 503, L161. Pulsar observations.
ADS
- Gotthelf et al. 1999, ApJ, 514, L107. X-ray variability of central source.
ADS
- Oliva et al. 1999, A&A, 343, 943. ISO spectroscopy.
ADS
- Torii et al. 2000, ApJ, 534, L71. X-ray timing on pulsar, including glitch.
ADS
- Reynoso et al. 2004, PASA, 21, 82. ATCA at 1.4 GHz (50''), including HI absorption to central source.
ADS
- Russeil et al. 2005, A&A, 429, 497. Hα observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Paron 2006, PASA, 23, 69. CO and HCO+ observations of surroundings.
ADS
- De Luca 2006, Science, 313, 814. XMM-Newton observations of central source.
ADS
- De Luca 2007, Ap&SS, 308, 231. XMM-Newton observation of periodicity of central source.
ADS
- Matsumoto et al. 2007, PASJ, 59, S199. Suzaku observations.
ADS
- De Luca 2008, ApJ, 682, 1185. IR observations of central source.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Xing et al. 2014, ApJ, 781, 64. Fermi observations.
ADS
- Frank et al. 2015, ApJ, 810, 113. Chandra observations.
ADS
- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
ADS
- Rea et al. 2016, ApJ, 828, L13. Chandra, NuSTAR and Swift observations.
ADS
- Borghese et al. 2018, MNRAS, 478, 741. NuSTAR and Swift observations of central source.
ADS
Last updated: 9 Apr 2019
G332.4+0.1
MSH 16−51, Kes 32
- Right Ascension: 16 15 20
- Declination: −50 42
- Size (/arcmin): 15
- Type: S
- Flux density at 1 GHz (/Jy): 26
- Spectral Index: 0.5
Notes: Has been called G332.4+0.2.
- Radio: Distorted shell, with thermal jet and plume adjacent.
- Optical: Detected.
- X-ray: Shell, brightest to NW.
- Point sources: Pulsar nearby.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Roger et al. 1985, Nature, 316, 44. MOST at 843 MHz (44''×57'').
ADS
- Caraveo 1993, ApJ, 415, L111. Nearby pulsar.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×56'': S=29 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
ADS
- Brinkmann et al. 1999, A&A, 346, 599. ROSAT image of remnant and nearby pulsar.
ADS
- Vink et al. 2004, ApJ, 604, 693. Chandra observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 30 May 2014
G332.5−5.6
- Right Ascension: 16 43 20
- Declination: −54 30
- Size (/arcmin): 35
- Type: S
- Flux density at 1 GHz (/Jy): 2?
- Spectral Index: 0.7?
- Radio: Bipolar shell, with central emission also.
- Optical: Patchy filaments.
- X-ray: Emission from centre.
- Distance: Optical extinction suggests 3 kpc.
References:
- Reynoso & Green 2007, MNRAS, 375, 92. ATCA at 1.4 GHz (40'': S=1.90±0.15 Jy) and 2.4 GHz (90'': S=1.3±0.2 Jy) including polarisation, and 843 MHz (43''×53'') plus ROSAT observations.
ADS
- Stupar et al. 2007, MNRAS, 381, 377. Optical observations, plus ATCA at 1.4 GHz (58'') and 2.4 GHz (95'') including polarisation, and other observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
- Zhu et al. 2015, MNRAS, 452, 3470. Suzaku observations, and distance estimate.
ADS
- Suárez et al. 2015, A&A, 583, A84. XMM-Newton observations of central region.
ADS
- Ackermann et al. 2018, ApJS, 237, 32. Fermi observations.
ADS
Last updated: 9 Apr 2019
G335.2+0.1
- Right Ascension: 16 27 45
- Declination: −48 47
- Size (/arcmin): 21
- Type: S
- Flux density at 1 GHz (/Jy): 16
- Spectral Index: 0.5
- Radio: Well defined shell.
- Point sources: Old pulsar within remnant boundary.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=27.1 Jy) and Parkes 64-m at 5 GHz (4': S=8.6 Jy).
ADS
- Kaspi et al. 1996, AJ, 111, 2028. Pulsar observations.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×57'': S=16 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
Last updated: 3 Apr 2019
G336.7+0.5
- Right Ascension: 16 32 11
- Declination: −47 19
- Size (/arcmin): 14×10
- Type: S
- Flux density at 1 GHz (/Jy): 6
- Spectral Index: 0.5
- Radio: Irregular shell.
- Optical: Detected.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×60'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×58'': S=6.1 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 25 Apr 2014
G337.0−0.1
(CTB 33)
- Right Ascension: 16 35 57
- Declination: −47 36
- Size (/arcmin): 1.5
- Type: S
- Flux density at 1 GHz (/Jy): 1.5
- Spectral Index: 0.6?
Notes: This entry refers to a small (1.'5) SNR, not the larger previously catalogued G337.0−0.1. Has mistakenly been called G337.7−0.1.
- Radio: Shell, in a complex region.
- Point sources: Associated with a soft gamma repeater.
- Distance: Association with CTB 33 gives 11 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×58'': S=21 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant, including masers.
ADS
- Sarma et al. 1997, ApJ, 483, 335. ATCA at 1.4 GHz (12'') including HI, and 8.9 GHz (13''×15'') for recombination lines, clarifying extent of the remnant.
ADS
- Woods et al. 1999, ApJ, 519, L139. Soft gamma repeater observations.
ADS
- Hurley et al. 2000, ApJ, 528, L21. ASCA observations of soft gamma repeater.
ADS
- Brogan et al. 2000, ApJ, 537, 875. VLA at 1.7 GHz for OH Zeeman splitting.
ADS
- Castro et al. 2013, ApJ, 774, 36. Fermi observations.
ADS
Last updated: 23 May 2014
G337.2−0.7
- Right Ascension: 16 39 28
- Declination: −47 51
- Size (/arcmin): 6
- Type: S
- Flux density at 1 GHz (/Jy): 1.5
- Spectral Index: 0.4
- Radio: Shell, brighter in S.
- X-ray: Extended emission.
- Distance: HI absorption suggests 2.0 to 9.3 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=3.8 Jy) and Parkes 64-m at 5 GHz (4': S=0.70 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×58'': S=2.0 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Rakowski et al. 2001, ApJ, 548, 258. ASCA and ROSAT observations.
ADS
- Rakowski et al. 2006, ApJ, 646, 982. ATCA observations at 1.3 GHz (15'': S=1.55±0.05 Jy) and 5 GHz (15'': S=0.93±0.02 Jy), plus HI and Chandra observations.
ADS
- Yamaguchi et al. 2014, ApJ, 785, L27. Suzaku observations.
ADS
- Takata et al. 2016, PASJ, 68, S3. Suzaku observations.
ADS
Last updated: 13 May 2017
G337.2+0.1
- Right Ascension: 16 35 55
- Declination: −47 20
- Size (/arcmin): 3×2
- Type: ?
- Flux density at 1 GHz (/Jy): 1.5?
- Spectral Index: ?
- Radio: Not well defined.
- X-ray: Detected.
- Distance: Association with HI hole gives 14 kpc.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=1.6 Jy)
ADS
- Combi et al. 2005, A&A, 431, L9. ASCA and other observations.
ADS
- Aharonian et al. 2006, ApJ, 636, 777. HESS observations of nearby source.
ADS
- Combi et al. 2006, ApJ, 653, L41. XMM-Newton observations.
ADS
Last updated: 19 Feb 2009
G337.3+1.0
Kes 40
- Right Ascension: 16 32 39
- Declination: −46 36
- Size (/arcmin): 15×12
- Type: S
- Flux density at 1 GHz (/Jy): 16
- Spectral Index: 0.55
- Radio: Nearly complete shell.
References:
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=24.6 Jy) and Parkes 64-m at 5 GHz (4': S=7.2 Jy).
ADS
- Dickel & Milne 1976, AuJPh, 29, 435. Comparison of earlier Parkes 64-m maps at 2.7 GHz (8.'4) and 5 GHz (4.'4).
ADS
- Kesteven & Caswell 1987, A&A, 183, 118. MOST at 843 MHz (44''×61'').
ADS
- Milne et al. 1989, PASA, 8, 187. MOST at 843 MHz (43''×59'': S=14.8±3.0 Jy), and Parkes 64-m at 8.4 GHz (3': S=5.1±0.6 Jy), including polarisation.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=20 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G337.8−0.1
Kes 41
- Right Ascension: 16 39 01
- Declination: −46 59
- Size (/arcmin): 9×6
- Type: S
- Flux density at 1 GHz (/Jy): 15
- Spectral Index: 0.5
- Radio: Distorted shell.
- X-ray: Centrally brightened.
- Distance: HI absorption suggests 11 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=18 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA detection of compact OH emission.
ADS
- Caswell 2004, MNRAS, 349, 99. ATCA at 1.7 GHz, for associated OH masers.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- Kothes & Dougherty 2007, A&A, 468, 993. SGPS at 1.4 GHz including HI.
ADS
- Combi et al. 2008, A&A, 488, L25. XMM-Newton observations.
ADS
- Zhang et al. 2015, ApJ, 799, 103. XMM-Newton, Chandra and CO observations.
ADS
- Liu et al. 2015, ApJ, 809, 102. Fermi observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Qiao et al. 2016, ApJS, 227, 26. OH maser observations.
ADS
- Supan et al. 2018, A&A, 619, A108. CO, HI and Spitzer observations.
ADS
- Supan et al. 2018, A&A, 619, A109. Fermi observations and review of radio flux densities.
ADS
Last updated: 9 Apr 2019
G338.1+0.4
- Right Ascension: 16 37 59
- Declination: −46 24
- Size (/arcmin): 15?
- Type: S
- Flux density at 1 GHz (/Jy): 4?
- Spectral Index: 0.4
- Radio: Arc in NE, merging with thermal emission in S.
- Optical: Detected.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Zealey et al. 1979, A&AS, 38, 39. Optical detection.
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=3.8 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 28 Apr 2017
G338.3−0.0
- Right Ascension: 16 41 00
- Declination: −46 34
- Size (/arcmin): 8
- Type: C?
- Flux density at 1 GHz (/Jy): 7?
- Spectral Index: ?
- Radio: Irregular shell, in complex region.
- X-ray: Central X-ray source and nebula.
- Point sources: Central pulsar.
- Distance: HI observations suggest 8 to 13 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=7.4 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Aharonian et al. 2005, Science, 307, 1938. HESS detection.
ADS
- Aharonian et al. 2006, ApJ, 636, 777. HESS observations.
ADS
- Landi et al. 2006, ApJ, 651, 190. X-ray observations.
ADS
- Funk et al. 2007, ApJ, 662, 517. XMM-Newton observations.
ADS
- Lemiere et al. 2009, ApJ, 706, 1269. Chandra observations of central source and nebula.
ADS
- Slane et al. 2010, ApJ, 720, 266. Fermi observations.
ADS
- Castelletti et al. 2011, A&A, 536, A98. GMRT at 235 MHz (10''×26''), 610 MHz (5.''0×12.''6) and 1280 MHz (5.''0×6.''4), plus ATCA at 2.3 GHz (4.''3×4.''8).
ADS
- Gotthelf et al. 2014, ApJ, 788, 155. NuSTAR observations.
ADS
- Lemoine-Goumard et al. 2014, ApJ, 794, L16. Fermi observations.
ADS
- Abramowski et al. 2014, MNRAS, 439, 2828. HESS observations.
ADS
also see: Abramowski et al. 2014, MNRAS, 441, 3640. Erratum.
ADS
- Supan et al. 2016, A&A, 589, A51. SGPS HI and other observations.
ADS
- Lau et al. 2017, MNRAS, 464, 3757. CO and other molecular line observations, plus HI observations.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
- Xin et al. 2018, ApJ, 867, 55. Fermi observations.
ADS
Last updated: 9 Apr 2019
G338.5+0.1
- Right Ascension: 16 41 09
- Declination: −46 19
- Size (/arcmin): 9
- Type: ?
- Flux density at 1 GHz (/Jy): 12?
- Spectral Index: ?
- Radio: Circle of non-thermal emission in complex region, not well defined.
- Distance: HI absorption suggests 11 kpc.
References:
- Shaver & Goss 1970, AuJPA, 14, 133. Molonglo at 408 MHz (3') and Parkes 64-m at 5 GHz (4').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×59'': S=13 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Kothes & Dougherty 2007, A&A, 468, 993. SGPS at 1.4 GHz including HI.
ADS
- Abramowski et al. 2014, ApJ, 794, L1. HESS observations.
ADS
- Lau et al. 2017, MNRAS, 464, 3757. CO and other molecular line observations, plus HI observations.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
Last updated: 9 Apr 2019
G340.4+0.4
- Right Ascension: 16 46 31
- Declination: −44 39
- Size (/arcmin): 10×7
- Type: S
- Flux density at 1 GHz (/Jy): 5
- Spectral Index: 0.4
- Radio: Distorted shell, elongated east–west.
- Optical: Detected.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=8.2 Jy) and Parkes 64-m at 5 GHz (4': S=2.9 Jy).
ADS
- Caswell et al. 1983, MNRAS, 203, 595. FIRST at 1415 MHz (50'').
ADS
- Dubner et al. 1996, AJ, 111, 1304. VLA at 330 MHz (48''×75'': S=9.8±0.9 Jy) and 1.4 GHz (9''×27'': S=3.6±0.1 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×61'': S=5.9 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
Last updated: 25 Apr 2014
G340.6+0.3
- Right Ascension: 16 47 41
- Declination: −44 34
- Size (/arcmin): 6
- Type: S
- Flux density at 1 GHz (/Jy): 5?
- Spectral Index: 0.4?
- Radio: Incomplete shell.
- Optical: Possible associated filaments.
- Distance: HI absorption suggests 15 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=7.0 Jy) and Parkes 64-m at 5 GHz (4': S=2.8 Jy).
ADS
- Zealey et al. 1979, A&AS, 38, 39. Optical observations.
ADS
- Caswell et al. 1983, MNRAS, 203, 595. FIRST at 1415 MHz (50'').
ADS
- Dubner et al. 1996, AJ, 111, 1304. VLA at 330 MHz (48''×75'': S=9.2±0.9 Jy) and 1.4 GHz (9''×27'': S=5.8±0.1 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×61'': S=4.5 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
ADS
- Kothes & Dougherty 2007, A&A, 468, 993. SGPS at 1.4 GHz including HI.
ADS
Last updated: 22 Apr 2014
G341.2+0.9
- Right Ascension: 16 47 35
- Declination: −43 47
- Size (/arcmin): 22×16
- Type: C
- Flux density at 1 GHz (/Jy): 1.5?
- Spectral Index: 0.6?
- Radio: Incomplete shell, with extension to SW.
- Point sources: Pulsar in W, with wind nebula.
References:
- Frail et al. 1994, ApJ, 437, 781. VLA at 330 MHz (54''×116'': S=3.0±0.1 Jy) and 1.4 GHz (21''×25'': S=12.5±0.05 Jy).
ADS
- Giacani et al. 2001, AJ, 121, 3133. VLA at 1.4 and 4.9 GHz (25'') of pulsar wind nebula.
ADS
Last updated: 8 Nov 2001
G341.9−0.3
- Right Ascension: 16 55 01
- Declination: −44 01
- Size (/arcmin): 7
- Type: S
- Flux density at 1 GHz (/Jy): 2.5
- Spectral Index: 0.5
- Radio: Incomplete shell, brightest to NE.
References:
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=7.4 Jy) and Parkes 64-m at 5 GHz (4': S=1.7 Jy).
ADS
- Caswell et al. 1983, MNRAS, 203, 595. FIRST at 1415 MHz (50''), revision of previous flux densities.
ADS
- Dubner et al. 1996, AJ, 111, 1304. VLA at 1.4 GHz (11''×35'': S=2.2±0.1 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×62'': S=2.7 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
Last updated: 27 Jan 2004
G342.0−0.2
- Right Ascension: 16 54 50
- Declination: −43 53
- Size (/arcmin): 12×9
- Type: S
- Flux density at 1 GHz (/Jy): 3.5?
- Spectral Index: 0.4?
- Radio: Distorted shell.
References:
- Caswell et al. 1983, MNRAS, 203, 595. FIRST at 1415 MHz (50''), estimate S408 MHz=5 Jy, S5 GHz=2 Jy from previous maps.
ADS
- Dubner et al. 1996, AJ, 111, 1304. VLA at 1.4 GHz (11''×35'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×62'': S=3.5 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
Last updated: 1 Aug 2000
G342.1+0.9
- Right Ascension: 16 50 43
- Declination: −43 04
- Size (/arcmin): 10×9
- Type: S
- Flux density at 1 GHz (/Jy): 0.5?
- Spectral Index: ?
- Radio: Incomplete shell.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×63'': S=0.6 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G343.0−6.0
RCW 114
- Right Ascension: 17 25 00
- Declination: −46 30
- Size (/arcmin): 250
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Faint, poorly defined.
- Optical: Filamentary shell.
References:
- Walker & Zealey 2001, MNRAS, 325, 287. Optical observations, and review of earlier observations.
ADS
- Welsh et al. 2003, A&A, 403, 605. Optical spectroscopy.
ADS
- Casandjian & Grenier 2008, A&A, 489, 849. γ-ray observations.
ADS
- Kim et al. 2010, ApJ, 709, 823. UV observations.
ADS
Last updated: 22 Apr 2014
G343.1−2.3
- Right Ascension: 17 08 00
- Declination: −44 16
- Size (/arcmin): 32?
- Type: C?
- Flux density at 1 GHz (/Jy): 8?
- Spectral Index: 0.5?
- Radio: Incomplete shell?
- X-ray: Pulsar wind nebula.
- Point sources: Pulsar near edge, with wind nebula.
References:
- McAdam et al. 1993, Nature, 361, 516. MOST at 843 MHz (smoothed to 2').
ADS
- Frail et al. 1994, ApJ, 437, 781. VLA at 330 MHz (56''×111'': S=10.6 Jy) and 1.4 GHz (22''×27'') near pulsar.
ADS
- Becker et al. 1995, A&A, 298, 528. ROSAT of pulsar, and limit for remnant.
ADS
- Giacani et al. 2001, AJ, 121, 3133. VLA at 1.4, 4.9 and 8.5 GHz (25'') of pulsar wind nebula.
ADS
- Gotthelf et al. 2002, ApJ, 567, L125. Pulsar x-ray detection.
ADS
- Dodson & Golap 2002, MNRAS, 334, L1. ATCA at 1.4 GHz (47''×70'') including polarisation, and Chandra observations of pulsar wind nebula.
ADS
- Aharonian et al. 2005, A&A, 432, L9. HESS limit.
ADS
- Abramowski et al. 2011, A&A, 528, A143. HESS observations.
ADS
Last updated: 22 Apr 2014
G343.1−0.7
- Right Ascension: 17 00 25
- Declination: −43 14
- Size (/arcmin): 27×21
- Type: S
- Flux density at 1 GHz (/Jy): 7.8
- Spectral Index: 0.55
- Radio: Shell, with smaller thermal shell adjacent.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×63'': S8.5±0.6), plus Parkes 64-m at 4.5 GHz (S=3.9±0.6 Jy) and 8.55 GHz (S=2.4±0.5 Jy)
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
Last updated: 1 Aug 2000
G344.7−0.1
- Right Ascension: 17 03 51
- Declination: −41 42
- Size (/arcmin): 8
- Type: C?
- Flux density at 1 GHz (/Jy): 2.5?
- Spectral Index: 0.3?
- Radio: Asymmetric shell, with possible core.
- X-ray: Detected.
- Distance: HI absorption and association with features suggests 6.3 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=4.7 Jy) and Parkes 64-m at 5 GHz (4': S=1.3 Jy).
ADS
- Dubner et al. 1993, AJ, 105, 2251. VLA at 1.47 GHz (30''×43'': S=1.7±0.1 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×65'': S=2.5 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Yamauchi et al. 2005, PASJ, 57, 459. ASCA observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Giacani et al. 2011, A&A, 531, A138. VLA and ATCA at 1.4 GHz (5.''6×8''), ATCA at 5 GHz (10''×13'') and 8.4 GHz (5''×10''), plus XMM-Newton observations and HI from SGPS.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Yamaguchi et al. 2012, ApJ, 749, 137. Suzaku observations.
ADS
- Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy.
ADS
Last updated: 23 May 2014
G345.7−0.2
- Right Ascension: 17 07 20
- Declination: −40 53
- Size (/arcmin): 6
- Type: S
- Flux density at 1 GHz (/Jy): 0.6?
- Spectral Index: ?
- Radio: Poorly defined diffuse shell.
- Point sources: Old pulsar nearby.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×66'': S=0.7 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G346.6−0.2
- Right Ascension: 17 10 19
- Declination: −40 11
- Size (/arcmin): 8
- Type: S
- Flux density at 1 GHz (/Jy): 8?
- Spectral Index: 0.5?
- Radio: Irregular shell.
- X-ray: Centrally brightened, clumpy.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=14.9 Jy) and Parkes 64-m at 5 GHz (4': S=4.3 Jy).
ADS
- Dubner et al. 1993, AJ, 105, 2251. VLA at 1.47 GHz (31''×43'': S=8.1±0.9 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×67'': S=8.7 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA detection of compact OH emission.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Hewitt et al. 2009, ApJ, 694, 1266. Spitzer spectroscopy.
ADS
- Sezer et al. 2011, MNRAS, 415, 301. Suzaku observations.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Yamauchi et al. 2013, PASJ, 65, 6. Suzaku observations.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Pannuti et al. 2014, AJ, 147, 55. ASCA observations.
ADS
- Auchettl et al. 2017, ApJ, 847, 121. XMM-Newton observations.
ADS
Last updated: 9 Apr 2019
G347.3−0.5
RX J1713.7−3946
- Right Ascension: 17 13 50
- Declination: −39 45
- Size (/arcmin): 65×55
- Type: S?
- Flux density at 1 GHz (/Jy): 30?
- Spectral Index: ?
- Radio: Faint emission.
- X-ray: Non-thermal, limb-brightened to W, with central source.
- Point sources: Central X-ray source.
- Distance: Association with molecular clouds and X-ray observations imply 1.3 kpc.
References:
- Koyama et al. 1997, PASJ, 49, L7. ASCA of NW.
ADS
- Slane et al. 1999, ApJ, 525, 357. ASCA and other observations.
ADS
- Muraishi et al. 2000, A&A, 354, L57. γ-ray detection.
ADS
- Butt et al. 2001, ApJ, 562, L167. Associated γ-ray emission.
ADS
- Ellison et al. 2001, ApJ, 563, 191. ATCA at 1.4 GHz (36''×46''), and ASCA observations.
ADS
- Enomoto et al. 2002, Nature, 416, 823. γ-ray observations.
ADS
- Uchiyama et al. 2002, PASJ, 54, L73. ASCA observations.
ADS
- Uchiyama et al. 2003, A&A, 400, 567. Chandra spectroscopy.
ADS
- Pannuti et al. 2003, ApJ, 593, 377. ROSAT, ASCA and RXTE observations.
ADS
- Lazendic et al. 2003, ApJ, 593, L27. Chandra, XMM-Newton and other X-ray observations of central source.
ADS
- Fukui et al. 2003, PASJ, 55, L61. CO observations of surroundings.
ADS
- Cassam-Chenaï et al. 2004, A&A, 427, 199. XMM-Newton and other observations.
ADS
- Aharonian et al. 2004, Nature, 432, 75. HESS detection.
ADS
- Lazendic et al. 2004, ApJ, 602, 271. Chandra observations of parts, and ATCA at 1.4 GHz (36''×46'').
ADS
- Hiraga et al. 2005, A&A, 431, 953. XMM-Newton observations,
ADS
- Moriguchi et al. 2005, ApJ, 631, 947. CO observations of surroundings.
ADS
- Aharonian et al. 2007, A&A, 464, 235. HESS observations.
ADS
also see: Aharonian et al. 2011, A&A, 531, C1. Erratum.
ADS
- Uchiyama et al. 2007, Nature, 449, 576. Chandra multi-epoch observations for study of small-scale variability.
ADS
- Tanaka et al. 2008, ApJ, 685, 988. Suzaku observations.
ADS
- Takahashi et al. 2008, PASJ, 60, S131. Suzaku observations of SW.
ADS
- Mignani et al. 2008, A&A, 484, 457. Optical and IR observations of central source.
ADS
- Acero et al. 2009, A&A, 505, 157. XMM-Newton observations, plus other radio, IR and HESS observations.
ADS
- Sano et al. 2010, ApJ, 724, 59. CO observations of region.
ADS
- Maxted et al. 2012, MNRAS, 422, 2230. Molecular line observations.
ADS
also see: Maxted et al. 2013, MNRAS, 430, 2511. Erratum.
ADS
- Sano et al. 2013, ApJ, 778, 59. CO, SGPS HI and Suzaku observations.
ADS
- Federici et al. 2015, A&A, 577, A12. Fermi detection.
ADS
- Sano et al. 2015, ApJ, 799, 175. Suzaku observations.
ADS
- Katsuda et al. 2015, ApJ, 814, 29. XMM-Newton observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Tsuji & Uchiyama 2016, PASJ, 68, 108. Chandra observations of NW.
ADS
- Acero et al. 2017, A&A, 597, A106. XMM-Newton observations for proper motion studies.
ADS
- Okuno et al. 2018, PASJ, 70, 77. Chandra observations.
ADS
- Abdalla et al. 2018, A&A, 612, A6. HESS observations.
ADS
Last updated: 15 Apr 2019
G348.5−0.0
- Right Ascension: 17 15 26
- Declination: −38 28
- Size (/arcmin): 10?
- Type: S?
- Flux density at 1 GHz (/Jy): 10?
- Spectral Index: 0.4?
- Radio: Arc, overlapping G348.5+0.1.
References:
- Kassim et al. 1991, ApJ, 374, 212. VLA at 333 MHz (46''×53''), 1.4 GHz (18''×33'') and part at 5 GHz (2.''5×3.''9).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×69'': S=10.2 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant, including masers.
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
ADS
- Hewitt et al. 2009, ApJ, 694, 1266. Spitzer spectroscopy.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Pannuti et al. 2014, AJ, 147, 55. XMM-Newton upper limit.
ADS
Last updated: 5 Jun 2019
G348.5+0.1
CTB 37A
- Right Ascension: 17 14 06
- Declination: −38 32
- Size (/arcmin): 15
- Type: S
- Flux density at 1 GHz (/Jy): 72
- Spectral Index: 0.3
- Radio: Shell, poorly define to S and W, overlapping G348.5−0.0 in E.
- X-ray: Brighter to W.
- Distance: HI absorption indicates 8.0 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 75. Molonglo at 408 MHz (3': S=97 Jy).
ADS
- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.'4: S=43 Jy).
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Milne et al. 1979, MNRAS, 188, 437. FIRST at 1415 MHz (0.'8: S>50) and Parkes 64-m at 14.7 GHz (2.'2: S=18±5 Jy).
ADS
- Downes 1984, MNRAS, 210, 845. VLA at 1465 MHz (20''×45'').
ADS
- Kassim et al. 1991, ApJ, 374, 212. VLA at 333 MHz (46''×53''), 1.4 GHz (18''×33'') and part at 5 GHz (2.''5×3.''9).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×69'': S=71 Jy).
ADS
- Brogan et al. 2000, ApJ, 537, 875. VLA at 1.7 GHz for OH Zeeman splitting.
ADS
- Reynoso & Mangum 2000, ApJ, 545, 874. CO observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Aharonian et al. 2008, A&A, 490, 685. HESS observations.
ADS
- Castro & Slane 2010, ApJ, 717, 372. Fermi observations.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Sezer et al. 2011, MNRAS, 417, 1387. Suzaku observations.
ADS
- Tian & Leahy 2012, MNRAS, 421, 2593. SGPS HI absorption observations.
ADS
- Maxted et al. 2013, MNRAS, 434, 2188. Molecular line observations of region.
ADS
- Pannuti et al. 2014, AJ, 147, 55. XMM-Newton and Chandra observations.
ADS
- Yamauchi et al. 2014, PASJ, 66, 2. Suzaku observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 27 Jun 2017
G348.7+0.3
CTB 37B
- Right Ascension: 17 13 55
- Declination: −38 11
- Size (/arcmin): 17?
- Type: S
- Flux density at 1 GHz (/Jy): 26
- Spectral Index: 0.3
- Radio: Incomplete shell with faint eastern extensions.
- X-ray: Diffuse emission.
- Point sources: X-ray pulsar.
- Distance: HI absorption suggests 13 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 75. Molonglo at 408 MHz (3': S=34 Jy).
ADS
- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.'4: S=32 Jy).
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Milne et al. 1979, MNRAS, 188, 437. FIRST at 1415 MHz (0.'8: S>20) and Parkes 64-m at 14.7 GHz (2.'2: S=8±3 Jy).
ADS
- Downes 1984, MNRAS, 210, 845. VLA at 1465 MHz (20''×45'').
ADS
- Kassim et al. 1991, ApJ, 374, 212. VLA at 333 MHz (46''×53'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×69'': S=33 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
ADS
- Aharonian et al. 2006, ApJ, 636, 777. HESS detection.
ADS
- Aharonian et al. 2008, A&A, 486, 829. HESS and Chandra observations.
ADS
- Nakamura et al. 2009, PASJ, 61, S197. Suzaku and Chandra observations.
ADS
- Halpern & Gotthelf 2010, ApJ, 710, 941. Chandra detection of pulsar.
ADS
- Halpern & Gotthelf 2010, ApJ, 725, 1384. Chandra observations of pulsar.
ADS
- Tian & Leahy 2012, MNRAS, 421, 2593. SGPS HI observations.
ADS
- Xin et al. 2016, ApJ, 817, 64. Fermi observations.
ADS
Last updated: 13 May 2017
G349.2−0.1
- Right Ascension: 17 17 15
- Declination: −38 04
- Size (/arcmin): 9×6
- Type: S
- Flux density at 1 GHz (/Jy): 1.4?
- Spectral Index: ?
- Radio: Elongated shell, adjacent to bright HII region.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×70'': S=1.6 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant.
ADS
Last updated: 27 Aug 1996
G349.7+0.2
- Right Ascension: 17 17 59
- Declination: −37 26
- Size (/arcmin): 2.5×2
- Type: S
- Flux density at 1 GHz (/Jy): 20
- Spectral Index: 0.5
- Radio: Incomplete clumpy shell, with enhancement to the S.
- X-ray: Irregular shell, brighter to S and E.
- Distance: HI absorption indicates 11.5 kpc.
References:
- Becker & Kundu 1975, AJ, 80, 679. NRAO 140-ft at 10.6 GHz (3').
ADS
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=31.0 Jy) and Parkes 64-m at 5 GHz (4': S=9.1 Jy), no maps.
ADS
- Caswell et al. 1975, A&A, 45, 239. Parkes HI absorption.
ADS
- Shaver et al. 1985, Nature, 313, 113. VLA at 1.4 GHz (3.''4×14.''5).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×71'': S=22 Jy).
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant, including masers.
ADS
- Brogan et al. 2000, ApJ, 537, 875. VLA at 1.7 GHz for OH Zeeman splitting.
ADS
- Reynoso & Mangum 2001, AJ, 121, 347. CO observations of the vicinity.
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Slane et al. 2002, ApJ, 580, 904. ASCA observations.
ADS
- Dubner et al. 2004, A&A, 426, 201. CO observations of surroundings.
ADS
- Lazendic et al. 2005, ApJ, 618, 733. Chandra observations.
ADS
- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
ADS
- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
ADS
- Hewitt et al. 2009, ApJ, 694, 1266. Spitzer spectroscopy.
ADS
- Castro & Slane 2010, ApJ, 717, 372. Fermi observations.
ADS
- Lazendic et al. 2010, MNRAS, 409, 371. OH, CO and other molecular line observations of region.
ADS
- Andersen et al. 2011, ApJ, 742, 7. Spitzer observations.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Tian & Leahy 2014, ApJ, 783, L2. SGPS HI observations.
ADS
- Yasumi et al. 2014, PASJ, 66, 68. Suzaku observations.
ADS
- Abramowski et al. 2015, A&A, 574, A100. HESS observations.
ADS
also see: Abramowski et al. 2015, A&A, 580, C1. Corrigendum.
ADS
- Ergin et al. 2015, ApJ, 804, 124. Fermi and Suzaku observations.
ADS
- Rho et al. 2015, ApJ, 812, 44. Herschel observations.
ADS
- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Abdalla et al. 2018, A&A, 612, A1. HESS observations.
ADS
Last updated: 15 Apr 2019
G350.0−2.0
- Right Ascension: 17 27 50
- Declination: −38 32
- Size (/arcmin): 45
- Type: S
- Flux density at 1 GHz (/Jy): 26
- Spectral Index: 0.4
Notes: Incorporates the previously catalogued G350.0−1.8 in the NW.
- Radio: Shell, brightest in NW.
- Optical: Detected.
- X-ray: Brighter to NW.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=49.5 Jy) and Parkes 64-m at 5 GHz (4': S=13.6 Jy).
ADS
- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.'4).
ADS
- Gaensler 1998, ApJ, 493, 781. VLA and Parkes 64-m at 1.4 GHz (18''×21'': S=22.3±0.3 Jy), clarifying extent of remnant.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
- Karpova et al. 2016, MNRAS, 462, 3845. XMM-Newton observations.
ADS
Last updated: 13 May 2017
G350.1−0.3
- Right Ascension: 17 21 05
- Declination: −37 27
- Size (/arcmin): 4?
- Type: ?
- Flux density at 1 GHz (/Jy): 6?
- Spectral Index: 0.8?
- Radio: Several clumps of emission.
- X-ray: Diffuse emission, with compact source.
- Point sources: X-ray source.
- Distance: HI absorption indicates 4.5 to 10.7 kpc, possible interaction with molecular cloud indicates 4.5 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=10.7) and Parkes 64-m at 5 GHz (4': S=1.7).
ADS
- Salter et al. 1986, A&A, 162, 217. VLA at 1.5 (4''×10.''4) and 4.8 GHz (15''×35'') and 15 GHz (2''×5'').
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×71'')..
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Gaensler et al. 2008, ApJ, 680, L37. VLA at 4.8 GHz (5.''6×11.''4) plus XMM-Newton observations.
ADS
- Lovchinsky et al. 2011, ApJ, 731, 70. Chandra and Spitzer observations.
ADS
- Yasumi et al. 2014, PASJ, 66, 68. Suzaku observations.
ADS
Last updated: 5 May 2017
G351.0−5.4
- Right Ascension: 17 46 00
- Declination: −39 25
- Size (/arcmin): 30
- Type: S
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: ?
- Radio: Faint shell, brighter to E and W.
References:
- de Gasperin et al. 2014, A&A, 568, A107. GMRT at 325 MHz (89''×141''), plus other observations.
ADS
Last updated: 12 Jun 2017
G351.2+0.1
- Right Ascension: 17 22 27
- Declination: −36 11
- Size (/arcmin): 7
- Type: C?
- Flux density at 1 GHz (/Jy): 5?
- Spectral Index: 0.4
Notes: Has been called G351.3+0.2.
- Radio: Distorted shell, with possible flat-spectrum core.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=8.1 Jy) and Parkes 64-m at 5 GHz (4': S=3.1 Jy).
ADS
- Becker & Helfand 1988, AJ, 95, 883. VLA at 5 GHz (15''), and at 15 GHz of core.
ADS
- Dubner et al. 1993, AJ, 105, 2251. VLA at 1.47 GHz (32''×36'': S=4.8±0.2 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×73'': S=5.5 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
Last updated: 13 Aug 1998
G351.7+0.8
- Right Ascension: 17 21 00
- Declination: −35 27
- Size (/arcmin): 18×14
- Type: S
- Flux density at 1 GHz (/Jy): 10
- Spectral Index: 0.5?
- Radio: Elongated shell, adjacent to bright HII region.
- Point sources: Pulsar nearby.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×74'': S=11 Jy).
ADS
- Tian et al. 2007, MNRAS, 378, 1283. SGPS at 1.4 GHz (100'': S=8.4±0.7 Jy) including HI.
ADS
Last updated: 19 Feb 2009
G351.9−0.9
- Right Ascension: 17 28 52
- Declination: −36 16
- Size (/arcmin): 12×9
- Type: S
- Flux density at 1 GHz (/Jy): 1.8?
- Spectral Index: ?
- Radio: Asymmetric shell.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×73'': S=2.0 Jy).
ADS
Last updated: 21 Aug 1996
G352.7−0.1
- Right Ascension: 17 27 40
- Declination: −35 07
- Size (/arcmin): 8×6
- Type: S
- Flux density at 1 GHz (/Jy): 4
- Spectral Index: 0.6
- Radio: Distorted shell.
- X-ray: Detected.
- Distance: HI absorption indicates 6.8 to 8.4 kpc.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=9.6 Jy) and Parkes 64-m at 5 GHz (4': S=2.3 Jy).
ADS
- Caswell et al. 1983, MNRAS, 203, 595. FIRST at 1415 MHz (1.'1).
ADS
- Dubner et al. 1993, AJ, 105, 2251. VLA at 1.47 GHz (34'': S=3.4±0.4 Jy).
ADS
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×75'': S=4.4 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Kinugasa et al. 1998, PASJ, 50, 249. ASCA observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Giacani et al. 2009, A&A, 507, 841. VLA at 4.8 GHz (9''×12''), plus HI and XMM-Newton observations.
ADS
- Pannuti et al. 2014, ApJ, 782, 102. XMM-Newton and Chandra observations.
ADS
- Sezer & Gök 2014, ApJ, 790, 81. Suzaku observations.
ADS
Last updated: 5 May 2017
G353.6−0.7
- Right Ascension: 17 32 00
- Declination: −34 44
- Size (/arcmin): 30
- Type: S
- Flux density at 1 GHz (/Jy): 2.5?
- Spectral Index: ?
Notes: Has erroneously been called G353.6−0.37.
- Radio: Shell, brighter to S.
- X-ray: Patchy shell, brighter to E.
- Point sources: Central X-ray source.
- Distance: Various observations suggest 3.2 kpc.
References:
- Tian et al. 2008, ApJ, 679, L85. SGPS at 1.4 GHz (100''), plus 843 MHz (43'') and X-ray observations.
ADS
- Halpern & Gotthelf 2010, ApJ, 710, 941. XMM-Newton observations.
ADS
- Tian et al. 2010, ApJ, 712, 790. XMM-Newton, Suzaku and CO observations.
ADS
- Abramowski et al. 2011, A&A, 531, A81. HESS observations.
ADS
- Bamba et al. 2012, ApJ, 756, 149. Suzaku observations.
ADS
also see: Bamba et al. 2012, ApJ, 761, 80. Erratum.
ADS
- Klochkov et al. 2013, A&A, 556, A41. XMM-Newton and other X-ray observations.
ADS
- Fukuda et al. 2014, ApJ, 788, 94. HESS, SGPS HI and CO observations.
ADS
- Nayana et al. 2017, MNRAS, 467, 155. GMRT at 325 MHz (97''×135'') and 610 MHz (105''×150''), plus other observations.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
- Doroshenko et al. 2017, A&A, 608, A23. XMM-Newton observations.
ADS
- Condon et al. 2017, ApJ, 851, 100. Fermi observations.
ADS
- Guo et al. 2018, ApJ, 853, 2. Fermi observations.
ADS
- Abdalla et al. 2018, A&A, 612, A1. HESS observations.
ADS
- Maxted et al. 2018, MNRAS, 474, 662. CO and HI observations.
ADS
Last updated: 15 Apr 2019
G353.9−2.0
- Right Ascension: 17 38 55
- Declination: −35 11
- Size (/arcmin): 13
- Type: S
- Flux density at 1 GHz (/Jy): 1?
- Spectral Index: 0.5?
- Radio: Shell, with central double source.
References:
- Green 2001, MNRAS, 326, 283. VLA at 327 MHz (2.'7×3.'0) and 1.4 GHz (36''×42''), plus 8.4 GHz (6.''1×8.''4) of central source only.
ADS
Last updated: 8 Nov 2001
G354.1+0.1
- Right Ascension: 17 30 28
- Declination: −33 46
- Size (/arcmin): 15×3?
- Type: C?
- Flux density at 1 GHz (/Jy): ?
- Spectral Index: varies
Notes: Is this a SNR?
- Radio: Elongated N–S.
- Point sources: Pulsar at S tip.
References:
- Frail et al. 1994, ApJ, 437, 781. VLA at 330 MHz (47''×99'') and 1.4 GHz (8.''8×21'').
ADS
- Ajello et al. 2016, ApJ, 819, 44. Fermi observations.
ADS
Last updated: 4 Jun 2017
G354.8−0.8
- Right Ascension: 17 36 00
- Declination: −33 42
- Size (/arcmin): 19
- Type: S
- Flux density at 1 GHz (/Jy): 2.8?
- Spectral Index: ?
- Radio: Distorted shell.
References:
- Whiteoak & Green 1996, A&AS, 118, 329. MOST at 843 MHz (43''×78'': S=3.1 Jy).
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
ADS
Last updated: 1 Aug 2000
G355.4+0.7
- Right Ascension: 17 31 20
- Declination: −32 26
- Size (/arcmin): 25
- Type: S
- Flux density at 1 GHz (/Jy): 5?
- Spectral Index: ?
- Radio: Faint, incomplete shell.
References:
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×77'').
ADS
- Roy & Bhatnagar 2006, JPhCS, 54, 152. GMRT at 330 MHz (1': S=8.9±1.3 Jy).
ADS
- Ajello et al. 2016, ApJ, 819, 44. Fermi observations.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 4 Jun 2017
G355.6−0.0
- Right Ascension: 17 35 16
- Declination: −32 38
- Size (/arcmin): 8×6
- Type: S
- Flux density at 1 GHz (/Jy): 3?
- Spectral Index: ?
- Radio: Well defined shell.
- X-ray: Centrally brightened.
References:
- Gray 1994, MNRAS, 270, 847. MOST at 843 MHz (43''×80'': S=2.6 Jy).
ADS
- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
ADS
- Roy & Bhatnagar 2006, JPhCS, 54, 152. GMRT at 330 MHz (1': S=3.3±0.5 Jy).
ADS
- Marquez-Lopez & Phillips 2010, MNRAS, 407, 94. Mid-IR observations.
ADS
- Minami et al. 2013, PASJ, 65, 99. Suzaku observations.
ADS
Last updated: 25 Apr 2014
G355.9−2.5
- Right Ascension: 17 45 53
- Declination: −33 43
- Size (/arcmin): 13
- Type: S
- Flux density at 1 GHz (/Jy): 8
- Spectral Index: 0.5
- Radio: Distorted shell, brightest to SE.
References:
- Clark et al. 1975, AuJPA, 37, 1. Molonglo at 408 MHz (3': S=12.3 Jy) and Parkes 64-m at 5 GHz (4': S=3.4 Jy).
ADS
- Dubner et al. 1993, AJ, 105, 2251. VLA at 1.47 GHz (32''×34'': S=5.0±0.3 Jy).
ADS
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×77'').
ADS
- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
ADS
- Marquez-Lopez & Phillips 2010, MNRAS, 407, 94. Mid-IR observations.
ADS
Last updated: 25 Apr 2014
G356.2+4.5
- Right Ascension: 17 19 00
- Declination: −29 40
- Size (/arcmin): 25
- Type: S
- Flux density at 1 GHz (/Jy): 4
- Spectral Index: 0.7
Notes: Has been called G356.2+4.4.
- Radio: Faint shell.
References:
- Duncan et al. 1995, MNRAS, 277, 36. Parkes 64-m at 2.4-GHz (10.'4).
ADS
- Bhatnagar 2000, MNRAS, 317, 453. GMRT at 327 MHz (1.'5×3': S=8.1±1.7 Jy), and NVSS at 1.4 GHz.
ADS
Last updated: 27 Apr 2014
G356.3−1.5
- Right Ascension: 17 42 35
- Declination: −32 52
- Size (/arcmin): 20×15
- Type: S
- Flux density at 1 GHz (/Jy): 3?
- Spectral Index: ?
- Radio: Double arc.
References:
- Gray 1994, MNRAS, 270, 847. MOST at 843 MHz (43''×79'': S=2.8 Jy).
ADS
- Bhatnagar 2002, MNRAS, 332, 1. GMRT at 327 MHz (0.'8×1.'7: S=5.7±0.2).
ADS
Last updated: 20 May 2014
G356.3−0.3
- Right Ascension: 17 37 56
- Declination: −32 16
- Size (/arcmin): 11×7
- Type: S
- Flux density at 1 GHz (/Jy): 3?
- Spectral Index: ?
Notes: Has been suggested this part of a larger SNR.
- Radio: Diffuse emission.
References:
- Gray 1994, MNRAS, 270, 847. MOST at 843 MHz (43''×81'': S=2.6 Jy).
ADS
- Roy & Pramesh Rao 2002, MNRAS, 329, 775. GMRT at 330 MHz (2.'7×4.'8).
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
Last updated: 13 May 2017
G357.7−0.1
MSH 17−39
- Right Ascension: 17 40 29
- Declination: −30 58
- Size (/arcmin): 8×3?
- Type: ?
- Flux density at 1 GHz (/Jy): 37
- Spectral Index: 0.4
Notes: Has been suggested that this is not a SNR.
- Radio: Multiple arcs and filaments, brighter to NW `head'.
- X-ray: Detected from NW `head', and SW `tail'.
- Distance: HI absorption suggests beyond Galactic Centre.
References:
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3': S=54.2 Jy) and Parkes 64-m at 5 GHz (4': S=18.5 Jy).
ADS
- Milne & Dickel 1975, AuJPh, 28, 209. Parkes 64-m at 5 GHz (4.'4: S=14.6 Jy).
ADS
- Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.'6).
ADS
- Caswell et al. 1980, MNRAS, 190, 881. FIRST at 1415 MHz (50'').
ADS
- Weiler & Panagia 1980, A&A, 90, 269. Effelsberg 100-m at 9 GHz (1.'5) (private communication from Baker).
ADS
- Shaver et al. 1985, Nature, 313, 113. VLA at 1.4 GHz (3.''8×10.''9) and 5 GHz (12''×26'').
ADS
- Becker & Helfand 1985, Nature, 313, 115. VLA at 1.4 GHz and 5 GHz.
ADS
- Helfand & Becker 1985, Nature, 313, 118. Suggest it is not a SNR.
ADS
- Shaver et al. 1985, A&A, 147, L23. Observations of peripheral compact source.
ADS
- Caswell et al. 1989, PASA, 8, 184. MOST at 843 MHz (43''×83'').
ADS
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×84'').
ADS
- Stewart et al. 1994, ApJ, 432, L39. ATCA at 4.79 and 5.84 GHz (12''×22'') and Effelsberg 100-m at 10.6 GHz (1'), including polarisation.
ADS
- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant, including masers.
ADS
- Yusef-Zadeh et al. 1999, ApJ, 527, 172. VLA of nearby OH masers.
ADS
- LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''×43'').
ADS
also see: LaRosa et al. 2000, AJ, 119, 3145. Erratum.
ADS
- Brogan et al. 2000, ApJ, 537, 875. VLA at 1.7 GHz for OH Zeeman splitting.
ADS
- Brogan & Goss 2003, AJ, 125, 272. VLA at 1.4 GHz (11.''4×13.''6), including HI, and 8.3 GHz (6.''8×14.''3) recombination line observation of HII region.
ADS
- Gaensler et al. 2003, ApJ, 594, L35. Chandra detection.
ADS
- Lazendic et al. 2003, AN, 324 (No S1), 157. Molecular line observations.
ADS
- Burton et al. 2004, MNRAS, 348, 638. IR and radio observations of HII region.
ADS
- Lazendic et al. 2004, MNRAS, 354, 393. IR and molecular line observations.
ADS
- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
ADS
- Phillips et al. 2009, MNRAS, 397, 1215. Observations of interactions with surroundings.
ADS
- Castro et al. 2013, ApJ, 774, 36. Fermi observations.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Acero et al. 2016, ApJS, 224, 8. Fermi observations.
ADS
- Qiao et al. 2018, ApJS, 239, 15. OH maser observations.
ADS
Last updated: 9 Apr 2019
G357.7+0.3
- Right Ascension: 17 38 35
- Declination: −30 44
- Size (/arcmin): 24
- Type: S
- Flux density at 1 GHz (/Jy): 10
- Spectral Index: 0.4?
- Radio: Non-thermal shell in complex region.
References:
- Reich & Fürst 1984, A&AS, 57, 165. Effelsberg 100-m at 2.7 GHz (4.'3: S=7±1.5 Jy), S5 GHz=5.5±1.5 Jy from surveys.
ADS
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×84'').
ADS
- Yusef-Zadeh et al. 1999, ApJ, 527, 172. VLA of nearby OH masers.
ADS
- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
ADS
- Phillips & Marquez-Lugo 2010, MNRAS, 409, 701. Spitzer observations of region.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
ADS
- Rho et al. 2017, ApJ, 834, 12. Molecular line observations.
ADS
Last updated: 9 Apr 2019
G358.0+3.8
- Right Ascension: 17 26 00
- Declination: −28 36
- Size (/arcmin): 38
- Type: S
- Flux density at 1 GHz (/Jy): 1.5?
- Spectral Index: ?
- Radio: Faint shell.
References:
- Duncan et al. 1995, MNRAS, 277, 36. Parkes 64-m at 2.4-GHz (10.'4).
ADS
- Bhatnagar 2000, MNRAS, 317, 453. GMRT at 327 MHz (1.'3×2.'2: S=2.5±1.3 Jy), and NVSS at 1.4 GHz.
ADS
Last updated: 27 Apr 2014
G358.1+1.0
- Right Ascension: 17 37 00
- Declination: −29 59
- Size (/arcmin): 20
- Type: S
- Flux density at 1 GHz (/Jy): 2?
- Spectral Index: ?
Notes: Was erroneously called G358.1+0.1.
- Radio: Faint shell.
References:
- Gray 1994, MNRAS, 270, 847. MOST at 843 MHz (43''×77'').
ADS
- Roy & Bhatnagar 2006, JPhCS, 54, 152. GMRT at 330 MHz (1': S=6.0±2.5 Jy).
ADS
Last updated: 28 Apr 2017
G358.5−0.9
- Right Ascension: 17 46 10
- Declination: −30 40
- Size (/arcmin): 17
- Type: S
- Flux density at 1 GHz (/Jy): 4?
- Spectral Index: ?
- Radio: Shell, brighter to NE.
References:
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×77'').
ADS
- Roy & Bhatnagar 2006, JPhCS, 54, 152. GMRT at 330 MHz (1': S=8.0±2.5 Jy).
ADS
Last updated: 16 Mar 2009
G359.0−0.9
- Right Ascension: 17 46 50
- Declination: −30 16
- Size (/arcmin): 23
- Type: S
- Flux density at 1 GHz (/Jy): 23
- Spectral Index: 0.5
- Radio: Incomplete shell.
- Optical: Detected.
- X-ray: Partial shell.
References:
- Reich et al. 1988, IAUCo, 101, 293. Summary of parameters.
ADS
- Reich et al. 1990, A&AS, 85, 633. Effelsberg 100-m at 2.7 GHz (4.'3).
ADS
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×86'').
ADS
- LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''×43'').
ADS
also see: LaRosa et al. 2000, AJ, 119, 3145. Erratum.
ADS
- Bamba et al. 2000, PASJ, 52, 259. ASCA observations.
ADS
- Yusef-Zadeh et al. 2004, ApJS, 155, 421. VLA at 1.4 GHz (8.''4×12.''8) of part.
ADS
- Bamba et al. 2009, ApJ, 691, 1854. Suzaku observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
- Ponti et al. 2015, MNRAS, 453, 172. XMM-Newton observations.
ADS
- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
Last updated: 3 Apr 2019
G359.1−0.5
- Right Ascension: 17 45 30
- Declination: −29 57
- Size (/arcmin): 24
- Type: S
- Flux density at 1 GHz (/Jy): 14
- Spectral Index: 0.4?
Notes: Has been called G359.10−0.5.
- Radio: Non-thermal shell in complex region, crossed by the `snake'.
- Optical: Detected.
- X-ray: Centrally brightened.
- Point sources: Several compact radio sources near centre, OH masers around edge.
References:
- Downes et al. 1979, A&AS, 35, 1. From observations by Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.'6: S=13 Jy).
ADS
- Reich & Fürst 1984, A&AS, 57, 165. Effelsberg 100-m at 2.7 GHz (4.'3: S=10±1.5 Jy) and 4.8 GHz (2.'4: S=8.1±0.5 Jy).
ADS
- Uchida et al. 1992, ApJ, 398, 128. VLA at 1.5 GHz (10''×11''), and observations of nearby molecular material.
ADS
- Uchida et al. 1992, AJ, 104, 1533. VLA at 1.4 GHz.
ADS
- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×85'').
ADS
- Yusef-Zadeh et al. 1995, Science, 270, 1801. VLA at 1.4 GHz (31''×33''), and 1.7 GHz for OH survey.
ADS
- LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24''×43'').
ADS
also see: LaRosa et al. 2000, AJ, 119, 3145. Erratum.
ADS
- Bamba et al. 2000, PASJ, 52, 259. ASCA observations.
ADS
- Lazendic et al. 2002, MNRAS, 331, 537. Observations of shocked molecular gas where the `snake' crosses the remnant.
ADS
- Yusef-Zadeh et al. 2004, ApJS, 155, 421. VLA at 1.4 GHz (8.''4×12.''8).
ADS
- Aharonian et al. 2008, A&A, 483, 509. XMM-Newton and HESS observations.
ADS
- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
ADS
- Bamba et al. 2009, ApJ, 691, 1854. Suzaku observations.
ADS
- Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations.
ADS
- Ohnishi et al. 2011, PASJ, 63, 527. Suzaku observations.
ADS
- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
ADS
- Ponti et al. 2015, MNRAS, 453, 172. XMM-Newton observations.
ADS
- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
ADS
- Hui et al. 2016, MNRAS, 457, 4262. Fermi observations of region.
ADS
- de Wilt et al. 2017, MNRAS, 468, 2093. Molecular line observations of region.
ADS
- Qiao et al. 2018, ApJS, 239, 15. OH maser observations.
ADS
Last updated: 9 Apr 2019
G359.1+0.9
- Right Ascension: 17 39 36
- Declination: −29 11
- Size (/arcmin): 12×11
- Type: S
- Flux density at 1 GHz (/Jy): 2?
- Spectral Index: ?
- Radio: Shell, brightest in E.
References:
- Gray 1994, MNRAS, 270, 847. MOST at 843 MHz (43''×88'': S=4.3 Jy).
ADS
- Roy & Bhatnagar 2006, JPhCS, 54, 152. GMRT at 330 MHz (1': S=4.3±1.0 Jy).
ADS
- Law et al. 2008, ApJS, 177, 515. VLA at 1.4 GHz (10.''9×15.''9: S=1.3±0.5 Jy).
ADS
Last updated: 19 Feb 2009
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Tech Wizards
Hello Earthians! Thank you for showing interest in knowing about us.
Techwizards aim towards providing easy on pocket and yet proffesionalism in technical support.
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Feta Scrambled Eggs
Description
A very TASTY way to add zip to boring scrambled eggs.
Ingredients
- 1 tablespoon butter
- ¼ cup chopped onion
- 4 eggs, beaten
- ¼ cup chopped tomatoes
- 2 tablespoons crumbled feta cheese
- salt and pepper to taste
Steps
- Melt butter in a skillet over medium heat. Saute onions until translucent. Pour in eggs. Cook, stirring occasionally to scramble. When eggs appear almost done, stir in chopped tomatoes and feta cheese, and season with salt and pepper. Cook until cheese is melted.
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The Davis Sailing Team is a diverse group of university students with one thing in common: sailing. Although many of us also enjoy hiking, backpacking, fancy food (just wait, you’ll understand), flying, etc. If you haven’t sailed before, don't worry! Regardless of your skill level, we’ll do our best to train you to be a competitive dinghy sailor. As a member, you will be a fractional-owner of our 7 sailboats and equipment, with unlimited sailing access at the Lake Washington Sailing Club in West Sacramento and access to some of the best sailing instructors available for free: your fellow teammates!
If you are a current student and in good standing at University of California, Davis you are eligible to join the team. You do not need prior experience to join but you must know how to swim. You must also be a member of our host sailing club, Lake Washington Sailing Club (LWSC), which entitles you to many other benefits. Don't worry about not being a LWSC member, the team will assist you with this application process. If you are an undergraduate student you will be eligible to sail in inter-collegiate and club events. However, if you are a graduate student, you can only compete in club events. However, everyone is encouraged to come to practice!
The Davis Sailing Team has tri-annual quarterly dues of $140. This includes all regatta expenses. For graduate students, community members and alumni, dues are $50 per quarter. In addition, we offer reduced dues of $50 for undergraduates in their first quarter on the team who will not be attending regattas, or for any undergraduate who joins or renews when there are no more regattas scheduled in the quarter. Have finanical concerns? Don't hesitate to talk to us! We'll do our best to work something out.


| Interface | Description |
|---|---|
| VisualizationChangeListener |
| Class | Description |
|---|---|
| AbstractOscilloscope |
Base abstract oscilloscope class.
|
| AbstractSpectrumAnalyzer |
An abstract class that serves as a base class for all spectrum analyzers.
|
| AbstractVisualization |
Visualization base class.
|
| FullColorSpectrogram |
Renders a spectrogram covering the full frequency range provided by the FFT.
|
| FullSpectrogram |
Renders a spectrogram covering the full frequency range provided by the FFT.
|
| FullSpectrum |
Shows a magnitude vs.
|
| OscilloscopeLines |
Oscilloscope lines.
|
| PianoRoll |
Renders a spectrogram displaying 9 octaves of musical notes.
|
| QuarterColorSpectrogram |
Renders a quarter-spectrogram.
|
| QuarterSpectrogram |
Renders a quarter-spectrogram.
|
| QuarterSpectrum |
Shows a magnitude vs.
|
| SimpleOscilloscope |
Simple oscilloscope.
|
| SpectrumBars |
Renders a spectrum analyzer.
|
| Stereograph |
Early high-end high-fidelity audio systems often had a display called a
“stereograph”.
|
| StereoOscilloscope |
Stereo oscilloscope.
|
| StereoWaveform |
This visualization shows the time-waveform of the input audio signal.
|
| VisualizationEvent | |
| VisualizationPanel | |
| VolumeMeter | |
| WaterBalloons |
Shows three hanging water balloons bouncing with the music.
|
| Waveform |
This visualization shows a representation of the time-waveform of the input
audio signal.
|
| WhiteFullSpectrum |
This is a version of the FullSpectrum visualization specifically designed to
allow direct comparison between the usual spectrum and a whitened spectrum.
|
| WhiteQuarterSpectrum |
This is a version of the QuarterSpectrum visualization specifically designed
to allow direct comparison between the usual spectrum and a whitened spectrum.
|


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Harry Styles Wants to Take Next Role as James Bond
Agent 007 has had many faces over the 57-year cinematic history of Ian Fleming's jet-setting British spy. The first film, “Dr. No” was released in 1962, while the last, “Spectre”, hit movie screens around the world in 2015. In total, 26 films were shot, and the honour of playing the martini-drinking man of mystery has fallen to 7 actors.
Harry Styles, a 25-year-old singer formerly of the UK boy band One Direction recently disclosed that he'd love to replace Daniel Craig as the the next James Bond.
"I grew up watching those. You know, I loved him when I was a kid. So I think it's kind of everyone's dream a little bit, right?" Harry said, speaking to Hits Radio about the next Bond.
However, at the moment, he is focused on his music career; his new single Lights Up was among the UK's top 10 singles last week.
“For me it’s a very uplifting song. It’s very liberating,” he said.
In any event, origins stories are popular these days and Harry Styles could be perfectly suited to play a young Agent 007. It may seem like a stretch, but Doctor Who is a woman now, so you never know.
Harry Edward Styles was born on the first of February, 1994 in England; the British singer and actor shot to stardom with the band One Direction and his success on The X Factor in 2010.


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