Note: this is
an archived version which has been superseded. The current SNR
catalogue is at
https://www.mrao.cam.ac.uk/surveys/snrs/
G31.9+0.0
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title/keyword/abstract
3C391
- Right Ascension: 18 49 25
- Declination: −00 55
- Size (/arcmin): 7×5
- Type: S
- Flux density at 1 GHz (/Jy): 25
- Spectral Index: varies
- Radio: Shell, brightest in NW, with low frequency turnover.
- X-ray: Diffuse with central core.
- Distance: HI absorption and CO association suggests 7.1 kpc, as does H_2 emission.
References:
- Radhakrishnan et al. 1972, ApJS, 24, 49. HI absorption.
ADS
- Becker & Kundu 1975, AJ, 80, 679. NRAO 140-ft at 10.6 GHz (3').
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- Green et al. 1975, A&A, 44, 187. Effelsberg 100-m at 15 GHz (58'': S>1.6).
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- Becker & Kundu 1976, ApJ, 204, 427. NRAO interferometer at 2.7 GHz (20''×23'') and 8 GHz (9''×24''), plus review of flux densities.
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- Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.'6).
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- Goss et al. 1979, A&A, 78, 75. FIRST at 1.4 GHz (54''×66'': S=20±2 Jy) and Effelsberg 100-m at 10.7 GHz (77'': S=7.5±0.8 Jy).
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- Wang & Seward 1984, ApJ, 279, 705. Einstein observations.
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- Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.'4×3.'7: S=44.8 Jy).
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- Reynolds & Moffett 1993, AJ, 105, 2226. VLA at 1.4 GHz (6''), including possible associated CO.
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- Moffett & Reynolds 1994, ApJ, 425, 668. VLA at 330 MHz (smoothed to 30'': S=38.5±0.5 Jy) 1.46 GHz (6.''7) and 4.85 GHz (6.''2×6.''4), including spectral index and polarisation studies.
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- Frail et al. 1996, AJ, 111, 1651. OH emission near remnant, including masers.
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- Gorham et al. 1996, ApJ, 458, 257. Pulsar search.
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- Reach & Rho 1996, A&A, 315, L277. ISO spectroscopy.
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- Rho & Petre 1996, ApJ, 467, 698. ROSAT observations.
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- Wilner et al. 1998, AJ, 115, 247. CO observations of surroundings.
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- Reach & Rho 1998, ApJ, 507, L93. ISO observations.
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- Reach & Rho 1999, ApJ, 511, 836. CO, HCO+ and CS observations of surroundings.
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- Reach & Rho 2000, ApJ, 544, 843. ISO observations of interactions with surroundings.
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also see: Reach & Rho 2001, ApJ, 558, 943. Erratum.
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- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
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- Chen & Slane 2001, ApJ, 563, 202. ASCA observations.
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- Reach et al. 2002, ApJ, 564, 302. Observations of shocked molecular species.
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- Chen et al. 2004, ApJ, 616, 885. Chandra observations.
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- Brogan et al. 2005, AJ, 130, 148. VLA at 74 MHz, 330 MHz and 1.5 GHz (70'').
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- Kawasaki et al. 2005, ApJ, 631, 935. ASCA observations.
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- Reach et al. 2006, AJ, 131, 1479. Spitzer observations.
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- Neufeld et al. 2007, ApJ, 664, 890. Spitzer observations.
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- Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers.
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- Castro & Slane 2010, ApJ, 717, 372. Fermi observations.
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- Yuan & Neufeld 2011, ApJ, 726, 76. Spitzer observations.
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- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.'5: S=8.9±0.6 Jy) including polarisation and review of flux densities.
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- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
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- Neufeld et al. 2014, ApJ, 781, 102. Spitzer and Herschel IR spectroscopy.
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- Ergin et al. 2014, ApJ, 790, 65. Fermi and Suzaku observations.
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- Gusdorf et al. 2014, IAUS, 296, 178. CO observations.
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- Su et al. 2014, IAUS, 296, 372. VGPS for HI absorption.
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- Lee et al. 2014, MNRAS, 443, 2650. [FeII] IR survey observations.
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- Sato et al. 2014, PASJ, 66, 124. Suzaku observations.
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- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
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- Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines.
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- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
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- Ranasinghe & Leahy 2017, ApJ, 843, 119. HI and CO observations.
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- Lee et al. 2019, AJ, 157, 123. [FeII] and H2 IR observations.
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- Chawner et al. 2020, MNRAS, 493, 2706. Herschel observations.
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- Lee et al. 2020, AJ, 160, 263. H2 IR observations.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18'': S=1.5 Jy) including polarisation, and Spitzer observations.
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- Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities.
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- Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20'') of region.
ADS
Last updated: 20 Dec 2022
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