G1.0−0.1
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- Right Ascension: 17 48 30
- Declination: −28 09
- Size (/arcmin): 8
- Type: S
- Flux density at 1 GHz (/Jy): 15
- Spectral Index: 0.6?
Notes: Has been called G1.05−0.1 and G1.05−0.15.
- Radio: Incomplete shell, to the S of Sgr D.
- X-ray: Possibly detected.
References:
- Downes et al. 1979, A&AS, 35, 1. Review of flux densities.
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- Anantharamaiah et al. 1991, MNRAS, 249, 262. VLA at 330 MHz (64″×100″: S=12.3 Jy).
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- Liszt 1992, ApJS, 82, 495. VLA at 1.6 GHz (13″×23″).
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- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43″×91″).
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- Mehringer et al. 1998, ApJ, 493, 274. VLA at 1.6 GHz (15″×28″) and 5 GHz, including masers observations.
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- Yusef-Zadeh et al. 1999, ApJ, 527, 172. VLA of nearby OH masers.
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- LaRosa et al. 2000, AJ, 119, 207. VLA at 333 MHz (24″×43″).
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also see: LaRosa et al. 2000, AJ, 119, 3145. Erratum.
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- Sidoli et al. 2001, A&A, 372, 651. BeppoSAX possible detection.
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- Yusef-Zadeh et al. 2004, ApJS, 155, 421. VLA at 1.4 GHz (30″).
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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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- Nobukawa et al. 2009, AdSpR, 43, 1045. Suzaku observations.
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- Marquez-Lugo & Phillips 2010, MNRAS, 407, 94. Mid-IR observations.
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- Pihlström et al. 2014, AJ, 147, 73. VLA search for methanol masers.
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- Ponti et al. 2015, MNRAS, 453, 172. XMM-Newton observations.
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- Froebrich et al. 2015, MNRAS, 454, 2586. H2 IR observations.
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- Ogbodo et al. 2020, MNRAS, 493, 199. OH maser observations.
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- Dokara et al. 2021, A&A, 651, A86. VLA at 4 to 8 GHz (18″) including polarisation, and Spitzer observations.
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Last updated: 20 Dec 2022
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