G0.0+0.0
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Sgr A East
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- Right Ascension: 17 45 44
- Declination: −29 00
- Size (/arcmin): 3.5×2.5
- Type: S
- Flux density at 1 GHz (/Jy): 100?
- Spectral Index: 0.8?
- Radio: Non-thermal shell, in complex region, interacting with molecular material to the W.
- X-ray: Diffuse emission, centrally peaked.
- Point sources: Compact X-ray/radio source.
References:
- Ekers et al. 1983, A&A, 122, 143. VLA at 1.4 GHz and 5 GHz (both 5″×8″), S1.4 GHz=77 Jy, S5.0 GHz=31 Jy.
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- Pedlar et al. 1989, ApJ, 342, 769. VLA at 332 MHz (12″), 1.4 GHz (1.″3×2.″5) and 5 GHz (1.″3×2.″5).
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- Mezger et al. 1989, A&A, 209, 337. Nearby molecular material.
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- Ho et al. 1991, Nature, 350, 309. VLA of NH3 emission from surroundings.
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- Anantharamaiah et al. 1991, MNRAS, 249, 262. VLA at 330 MHz (17″×33″).
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- Serabyn et al. 1992, ApJ, 395, 166. Nearby molecular material.
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- Gray 1994, MNRAS, 270, 835. MOST at 843 MHz (43″×88″).
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- Yusef-Zadeh & Mehringer 1995, ApJ, 452, L37. VLA of nearby H2O masers.
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- Yusef-Zadeh et al. 1999, ApJ, 512, 230. OH maser observations.
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- Coil & Ho 2000, ApJ, 533, 245. NH3 observations of surroundings.
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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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- Fatuzzo et al. 2001, ApJ, 549, 293. Electron–positron lines from the vicinity.
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- Yusef-Zadeh et al. 2001, ApJ, 560, 749. Observations of nearby molecular hydrogen.
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- Maeda et al. 2002, ApJ, 570, 671. Chandra observations.
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- Sakano et al. 2003, AN, 324 (No S1), 197. XMM-Newton observations.
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- Roy & Pramesh Rao 2004, MNRAS, 349, L25. GMRT at 620 MHz (6.′6×11.′4).
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- Sakano et al. 2004, MNRAS, 350, 129. XMM-Newton observations.
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- Yusef-Zadeh et al. 2004, ApJS, 155, 421. VLA at 1.4 GHz (1″×2.″2).
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- Park et al. 2005, ApJ, 631, 964. Chandra observations.
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- Aharonian et al. 2006, ApJ, 636, 777. H.E.S.S. detection.
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- Koyama et al. 2007, PASJ, 59, S237. Suzaku observations.
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- Lee et al. 2008, ApJ, 674, 247. Molecular H2 observations of surroundings.
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- Sjouwerman & Pihlström 2008, ApJ, 681, 1287. VLA at 1.7 GHz of OH masers.
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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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- Tsuboi & Miyazaki 2012, PASJ, 64, 111. CO observations of SW.
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- Minh et al. 2013, ApJ, 773, 31. NH3 observations of region.
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- Zhao et al. 2013, ApJ, 777, 146. VLA at 4.8 GHz (0.″5×0.″7), 5.5 GHz (0.″6×1.″6), and 8.3 GHz (1.″0×2.″0).
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- Nynka et al. 2013, ApJ, 778, L31. NuSTAR of compact X-ray source.
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- Pihlström et al. 2014, AJ, 147, 73. VLA observations of methanol masers.
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- Ponti et al. 2015, MNRAS, 453, 172. XMM-Newton observations.
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- Tsuboi et al. 2015, PASJ, 67, 109. CO observations of region.
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- Lau et al. 2015, Science, 348, 413. IR observations.
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- Ajello et al. 2016, ApJ, 819, 44. Fermi observations.
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- Yusef-Zadeh et al. 2016, ApJ, 819, 60. VLA at 1.5 GHz 0.″5×1.″4) and other frequencies.
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- McEwen et al. 2016, ApJ, 832, 129. CH3OH maser observations in region.
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- Qiao et al. 2018, ApJS, 239, 15. OH maser observations.
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- Ono et al. 2019, PASJ, 71, 52. Suzaku X-ray spectroscopy.
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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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- Zhou et al. 2021, ApJ, 908, 31. Chandra observations.
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- Tanaka et al. 2021, ApJ, 915, 79. [CI] sub-mm observations of surroundings.
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Last updated: 20 Dec 2022
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