G33.6+0.1
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Kes 79,
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4C00.70,
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HC13
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- Right Ascension: 18 52 48
- Declination: +00 41
- Size (/arcmin): 10
- Type: S
- Flux density at 1 GHz (/Jy): 20
- Spectral Index: 0.51
Notes: Has been called G33.7+0.0 and G33.7+0.05.
- Radio: Shell, with bright central region, in complex region.
- X-ray: Multiple shells and filaments.
- Point sources: Central X-ray pulsar.
- Distance: HI absorption suggests 7.8 or 3.5 kpc, and CO observations suggest 5.5 kpc.
References:
- Caswell et al. 1975, AuJPA, 37, 39. Molonglo at 408 MHz (3′: S=35.5 Jy) and Parkes 64-m at 5 GHz (4′: S=7.8 Jy).
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- Caswell et al. 1975, A&A, 45, 239. HI absorption.
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- Dickel & DeNoyer 1975, AJ, 80, 437. Arecibo S430 MHz=69±33 Jy.
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- Becker & Kundu 1975, AJ, 80, 679. NRAO 140-ft at 10.6 GHz (3′: S=6.8±1.5 Jy).
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- Angerhofer et al. 1977, A&A, 55, 11. NRAO 140-ft at 5 GHz (6.′8: S=11.4±1.1 Jy).
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- Caswell et al. 1981, MNRAS, 195, 89. FIRST at 1415 MHz (1′), plus observations of the nearby point source.
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- van Gorkom et al. 1982, MNRAS, 198, 757. WSRT HI absorption to nearby point source, possibly extragalactic.
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- Seaquist & Gilmore 1982, AJ, 87, 378. VLA observations of nearby source, plus Einstein observations.
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- Green 1989, MNRAS, 238, 737. OH absorption.
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- Frail & Clifton 1989, ApJ, 336, 854. VLA at 1.4 GHz (1′×2.′9), including HI absorption.
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- Velusamy et al. 1991, AJ, 102, 676. VLA at 327 MHz (1′), 1.5 (7″×14″) and 5 GHz (7″), including spectral comparison.
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- Green & Dewdney 1992, MNRAS, 254, 686. Observations of adjacent molecular material.
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- Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.′6×3.′8: S=34.8 Jy).
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- Seward & Velusamy 1995, ApJ, 439, 715. ROSAT observations.
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- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
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- Koralesky et al. 1998, AJ, 116, 1323. VLA search for OH emission.
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- Sugizaki et al. 2001, ApJS, 134, 77. ASCA survey observations.
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- Tsunemi & Enoguchi 2002, PASJ, 54, 735. ASCA observations.
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- Seward et al. 2003, ApJ, 584, 414. Chandra observations.
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- Stanimirović 2003, ApJ, 592, 953. Arecibo OH absorption.
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- Sun et al. 2004, ApJ, 605, 742. Chandra observations.
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- Gotthelf et al. 2005, ApJ, 627, 390. XMM-Newton pulsar detection.
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- Reach et al. 2006, AJ, 131, 1479. Spitzer possible detection.
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- Halpern et al. 2007, ApJ, 665, 1304. X-ray pulsar timing observations.
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- Giacani et al. 2009, A&A, 507, 841. VLA at 74 MHz (36″×39″: S=76±10 Jy), 324 MHz (13″: S=39±8 Jy) and 1.5 GHz (17″×19″: S=11.5±1.5 Jy), plus review of flux densities and XMM-Newton observations.
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- Sun et al. 2011, A&A, 536, A83. Urumqi 25-m at 5 GHz (9.′5: S=9.4±0.5 Jy) including polarisation and review of flux densities.
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- Auchettl et al. 2014, ApJ, 783, 32. Fermi detection.
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- Kilpatrick et al. 2016, ApJ, 816, 1. CO observations, including broad lines.
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- Zhou et al. 2016, ApJ, 831, 192. CO and other observations.
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- Sato et al. 2016, PASJ, 68, S8. Suzaku observations.
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- Ranasinghe & Leahy 2018, AJ, 155, 204. VGPS HI absorption observations.
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- Kuriki et al. 2018, ApJ, 864, 161. CO observations.
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- Mayer & Becker 2021, A&A, 651, A40. Multi-epoch Chandra observations for proper motion of compact source.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″: S=1.2 Jy) including polarisation, and Spitzer observations.
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- Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20″) of region.
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- Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy.
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- He et al. 2022, ApJ, 928, 89. Fermi observations.
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- Dokara et al. et al. 2023, A&A, 671, A145. VLA and Effelsberg 100-m at 6 GHz, including polarisation, plus other radio flux densities.
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Last updated: 19 Mar 2024
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