Note: this is an archived version which has been superseded. The current SNR catalogue is at http://www.mrao.cam.ac.uk/surveys/snrs/

G1.0−0.1

• 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. ADS
• Anantharamaiah et al. 1991, MNRAS, 249, 262. VLA at 330 MHz (64''×100'': S=12.3 Jy). ADS
• Liszt 1992, ApJS, 82, 495. VLA at 1.6 GHz (13''×23''). ADS
• Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43''×91''). ADS
• Mehringer et al. 1998, ApJ, 493, 274. VLA at 1.6 GHz (15''×28'') and 5 GHz, including masers observations. 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 (43''×24''). ADS
  also see: LaRosa et al. 2000, AJ, 119, 3145. Erratum. ADS
• Sidoli et al. 2001, A&A, 372, 651. BeppoSAX possible detection. ADS
• Yusef-Zadeh et al. 2004, ApJS, 155, 421. VLA at 1.4 GHz (30''). ADS
• Hewitt et al. 2008, ApJ, 683, 189. GBT at 1.6 and 1.7 GHz for OH masers. ADS
• Nobukawa et al. 2009, AdSpR, 43, 1045. Suzaku observations. ADS
• Marquez-Lopez & Phillips 2010, MNRAS, 407, 94. Mid-IR 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

Last updated: 4 Jun 2017

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