G4.5+6.8 ADS: search fulltext or title/keyword/abstract

Kepler, SN1604, 3C358

• Right Ascension: 17 30 42
• Declination: −21 29
• Size (/arcmin): 3
• Type: S
• Flux density at 1 GHz (/Jy): 19
• Spectral Index: 0.64

Notes: This is the remnant of Kepler's SN of AD1604.

Radio: Incomplete shell, brighter to the N.

Optical: Faint filaments.

X-ray: Shell, brighter to the N.

Distance: Optical expansion and proper motion indicates about 2.9 kpc, HI observations suggest 3.4 to 6.4 kpc.

References:

• van den Bergh & Kamper 1977, ApJ, 218, 617. Optical proper motions. ADS
• Leibowitz & Danziger 1983, MNRAS, 204, 273. Optical spectra. ADS
• White & Long 1983, ApJ, 264, 196. Einstein observations. ADS
• Matsui et al. 1984, ApJ, 287, 295. VLA at 1.4 (2.''5×3.''2) and 5 GHz (3.''2×4.''8) and Einstein image (5''). ADS
• Dickel et al. 1988, ApJ, 330, 254. VLA at 1.4 (1.''2×2.''3) and 5 GHz (0.''6×1.''0) at two epochs. ADS
• Smith et al. 1989, ApJ, 347, 925. EXOSAT observations. ADS
• Hatsukade et al. 1990, PASJ, 42, 279. X-ray spectrum. ADS
• Blair et al. 1991, ApJ, 366, 484. Optical imaging and spectroscopy. ADS
• Bandiera & van den Bergh 1991, ApJ, 374, 186. Optical changes. ADS
• van den Bergh & Pritchet 1991, PASP, 103, 194. Optical imaging. ADS
• Predehl & Schmitt 1995, A&A, 293, 889. ROSAT of dust scattered halo. ADS
• Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations. ADS
• Hughes 1999, ApJ, 527, 298. ROSAT and Einstein image comparison for expansion studies. ADS
• Reynoso & Goss 1999, AJ, 118, 926. VLA at 1.4 GHz (13''×23'') for HI studies. ADS
• Kinugasa & Tsunemi 1999, PASJ, 51, 239. ASCA observations. ADS
• Gerardy & Fesen 2001, AJ, 121, 2781. IR spectroscopy and imaging. ADS
• DeLaney et al. 2002, ApJ, 580, 914. VLA at 1.3 to 1.5 GHz and 5 GHz (7.''2) for spectral index studies. ADS
• Morgan et al. 2003, ApJ, 597, L33. Sub-mm dust observations. ADS
• Sollerman et al. 2003, A&A, 407, 249. Optical spectroscopy. ADS
• Cassam-Chenaï et al. 2004, A&A, 414, 545. XMM-Newton observations. ADS
• Bamba et al. 2005, ApJ, 621, 793. Chandra observations of rim. ADS
• Riesgo & López 2005, RMxAA, 41, 57. Optical observations of filament (previously classified as PN, H 2-12). ADS
• Blair et al. 2007, ApJ, 662, 998. Spitzer observations. ADS
• Reynolds et al. 2007, ApJ, 668, L135. Chandra observations. ADS
• Sankrit et al. 2008, AJ, 135, 538. HST observations. ADS
• Aharonian et al. 2008, A&A, 488, 219. H.E.S.S. upper limit. ADS
• Enomoto et al. 2008, ApJ, 683, 383. γ-ray upper limit. ADS
• Katsuda et al. 2008, ApJ, 689, 225. Chandra proper motion studies. ADS
• Vink et al. 2008, ApJ, 689, 231. Chandra proper motion studies. ADS
• Gomez et al. 2012, MNRAS, 420, 3557. Herschel IR dust observations. ADS
• Williams et al. 2012, ApJ, 755, 3. Spitzer spectroscopy. ADS
• Burkey et al. 2013, ApJ, 764, 63. Chandra observations. ADS
• Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy. ADS
• Park et al. 2013, ApJ, 767, L10. Suzaku observations. ADS
• Katsuda et al. 2015, ApJ, 808, 49. XMM-Newton, Chandra and Suzaku observations. ADS
• Sankrit et al. 2016, ApJ, 817, 36. HST for proper motion studies. ADS
• Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties). ADS
• Sato & Hughes 2017, ApJ, 845, 167. Chandra expansion studies. ADS
• Kasuga et al. 2018, PASJ, 70, 88. Chandra observations. ADS
• Sun & Chen 2019, ApJ, 872, 45. Chandra observations. ADS
• Weinberger et al. 2020, A&A, 638, A83. INTEGRAL observations. ADS
• Sato et al. 2020, ApJ, 890, 104. Chandra observations. ADS
• Millard et al. 2020, ApJ, 893, 98. Chandra spectroscopy. ADS
• Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities. ADS
• Xiang & Jiang 2021, ApJ, 908, 22. Fermi observations. ADS
• Kasuga et al. 2021, ApJ, 915, 42. XMM-Newton spectroscopy. ADS
• Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy. ADS
• Nagayoshi et al. 2021, PASJ, 73, 302. Suzaku observations. ADS

Last updated: 15 Dec 2022

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