G4.5+6.8
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Kepler,
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SN1604,
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3C358
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- 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.
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- Leibowitz & Danziger 1983, MNRAS, 204, 273. Optical spectra.
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- White & Long 1983, ApJ, 264, 196. Einstein observations.
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- 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″).
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- 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.
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- Smith et al. 1989, ApJ, 347, 925. EXOSAT observations.
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- Hatsukade et al. 1990, PASJ, 42, 279. X-ray spectrum.
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- Blair et al. 1991, ApJ, 366, 484. Optical imaging and spectroscopy.
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- Bandiera & van den Bergh 1991, ApJ, 374, 186. Optical changes.
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- van den Bergh & Pritchet 1991, PASP, 103, 194. Optical imaging.
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- Predehl & Schmitt 1995, A&A, 293, 889. ROSAT of dust scattered halo.
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- Green et al. 1997, AJ, 114, 2058. Parkes 64-m OH observations.
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- Hughes 1999, ApJ, 527, 298. ROSAT and Einstein image comparison for expansion studies.
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- Reynoso & Goss 1999, AJ, 118, 926. VLA at 1.4 GHz (13″×23″) for HI studies.
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- Kinugasa & Tsunemi 1999, PASJ, 51, 239. ASCA observations.
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- Gerardy & Fesen 2001, AJ, 121, 2781. IR spectroscopy and imaging.
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- DeLaney et al. 2002, ApJ, 580, 914. VLA at 1.3 to 1.5 GHz and 5 GHz (7.″2) for spectral index studies.
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- Morgan et al. 2003, ApJ, 597, L33. Sub-mm dust observations.
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- Sollerman et al. 2003, A&A, 407, 249. Optical spectroscopy.
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- Cassam-Chenaï et al. 2004, A&A, 414, 545. XMM-Newton observations.
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- Bamba et al. 2005, ApJ, 621, 793. Chandra observations of rim.
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- Riesgo & López 2005, RMxAA, 41, 57. Optical observations of filament (previously classified as PN, H 2-12).
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- Blair et al. 2007, ApJ, 662, 998. Spitzer observations.
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- Reynolds et al. 2007, ApJ, 668, L135. Chandra observations.
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- Sankrit et al. 2008, AJ, 135, 538. HST observations.
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- Aharonian et al. 2008, A&A, 488, 219. H.E.S.S. upper limit.
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- Enomoto et al. 2008, ApJ, 683, 383. γ-ray upper limit.
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- Katsuda et al. 2008, ApJ, 689, 225. Chandra proper motion studies.
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- Vink et al. 2008, ApJ, 689, 231. Chandra proper motion studies.
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- Gomez et al. 2012, MNRAS, 420, 3557. Herschel IR dust observations.
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- Williams et al. 2012, ApJ, 755, 3. Spitzer spectroscopy.
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- Burkey et al. 2013, ApJ, 764, 63. Chandra observations.
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- Yang et al. 2013, ApJ, 766, 44. Suzaku spectroscopy.
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- Park et al. 2013, ApJ, 767, L10. Suzaku observations.
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- Katsuda et al. 2015, ApJ, 808, 49. XMM-Newton, Chandra and Suzaku observations.
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- Sankrit et al. 2016, ApJ, 817, 36. HST for proper motion studies.
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- Koo et al. 2016, ApJ, 821, 20. Spitzer and Herschel flux densities (and comparison with X-ray properties).
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- Sato & Hughes 2017, ApJ, 845, 167. Chandra expansion studies.
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- Kasuga et al. 2018, PASJ, 70, 88. Chandra observations.
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- Sun & Chen 2019, ApJ, 872, 45. Chandra observations.
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- Weinberger et al. 2020, A&A, 638, A83. INTEGRAL observations.
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- Sato et al. 2020, ApJ, 890, 104. Chandra observations.
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- Millard et al. 2020, ApJ, 893, 98. Chandra spectroscopy.
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- Castelletti et al. 2021, A&A, 653, A62.VLA 74-MHz survey flux density, and other low-frequency radio flux densities.
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- Xiang & Jiang 2021, ApJ, 908, 22. Fermi observations.
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- Kasuga et al. 2021, ApJ, 915, 42. XMM-Newton spectroscopy.
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- Millard et al. 2021, ApJS, 257, 36. ISO far-IR spectroscopy.
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- Nagayoshi et al. 2021, PASJ, 73, 302. Suzaku observations.
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- Acero et al. 2022, A&A, 660, A129. Fermi observations.
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- H.E.S.S. Collaboration: Aharonian et al. 2022, A&A, 662, A65. H.E.S.S. observations.
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- Coffin et al. 2022, ApJ, 926, 84. Chandra proper motion study.
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Last updated: 5 Jan 2024
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