G32.8−0.1 ADS: search title/keyword/abstract or fulltext

Kes 78 ADS: search title/keyword/abstract or fulltext

• Right Ascension: 18 51 25
• Declination: −00 08
• Size (/arcmin): 22×15
• Type: S?
• Flux density at 1 GHz (/Jy): 12
• Spectral Index: 0.3

Notes: Part has been called G33.1−0.1.

Radio: Incomplete, elongated shell.

Optical: Detected.

X-ray: Patchy, elongated shell.

Distance: Association with CO and HI absorption indicate 4.8 kpc, H₂ emission suggests 5.4 kpc.

References:

• Velusamy & Kundu 1974, A&A, 32, 375. NRAO 300-ft et 2.7 GHz (5′: S=7.2±0.5 Jy). ADS
• Dickel & DeNoyer 1975, AJ, 80, 437. Arecibo at 430 MHz (S=19.0±15.5 Jy). ADS
• 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=12.8 Jy) and Parkes 64-m at 5 GHz (4′: S=7.7 Jy). ADS
• Altenhoff et al. 1979, A&AS, 35, 23. Effelsberg 100-m at 4.9 GHz (2.′6). ADS
• Kassim 1992, AJ, 103, 943. VLA at 327 MHz (3.′6×3.′8: S=31.3 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
• Stupar & Parker 2011, MNRAS, 414, 2282. Hα observations. ADS
• Zhou & Chen 2011, ApJ, 743, 4. XMM-Newton observations, plus CO 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
• Bamba et al. 2016, ApJ, 818, 63. Suzaku observations. ADS
• Miceli et al. 2017, A&A, 599, A45. XMM-Newton observations. ADS
• Ranasinghe & Leahy 2018, AJ, 155, 204. VGPS HI absorption observations. ADS
• Lee et al. 2019, AJ, 157, 123. [FeII] and H₂ IR observations. ADS
• Lee et al. 2020, AJ, 160, 263. H₂ IR observations. ADS
• Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″) including polarisation, and Spitzer observations. ADS
• Sofue et al. 2021, ApJS, 253, 17. Nobeyama 45-m CO observations (20″) of region. ADS
• 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. ADS

Last updated: 19 Mar 2024

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