とも座CP星
出典: フリー百科事典『ウィキペディア(Wikipedia)』 (2022/11/22 14:34 UTC 版)
とも座CP星(ともざCPせい、CP Puppis、CP Pup)あるいは1942年のとも座新星は、1942年にとも座に出現した新星である。観測史上特に明るい古典新星の一つで、極大時には明るさが0.7等級にまで増光した[1]。また、極大後に暗くなるのも非常に早い、「速い新星」であり、新星爆発前後の明るさの差も非常に大きい、稀有な新星である[7]。
注釈
出典
- ^ a b c d Strope, Richard J.; Schaefer, Bradley E.; Henden, Arne A. (2010-07), “Catalog of 93 Nova Light Curves: Classification and Properties”, Astronomical Journal 140 (1): 34-62, Bibcode: 2010AJ....140...34S, doi:10.1088/0004-6256/140/1/34
- ^ Samus, N. N.; et al. (2009-01), “General Catalogue of Variable Stars”, VizieR On-line Data Catalog: B/gcvs, Bibcode: 2009yCat....102025S
- ^ a b c d e f g “CP Pup -- Nova”. SIMBAD. CDS. 2019年9月13日閲覧。
- ^ a b Downes, Ronald A.; Duerbeck, Hilmar W. (2000-10), “Optical Imaging of Nova Shells and the Maximum Magnitude-Rate of Decline Relationship”, Astronomical Journal 120 (4): 2007-2037, Bibcode: 2000AJ....120.2007D, doi:10.1086/301551
- ^ a b Pearson, K. J. (2006-09), “Superhumps: confronting theory with observation”, Monthly Notices of the Royal Astronomical Society 371 (1): 235-244, Bibcode: 2006MNRAS.371..235P, doi:10.1111/j.1365-2966.2006.10631.x
- ^ a b c Schaefer, Bradley E.; Collazzi, Andrew C. (2010-05), “Novae with Long-lasting Supersoft Emission that Drive a High Accretion Rate”, Astronomical Journal 139 (5): 1831-1843, Bibcode: 2010AJ....139.1831S, doi:10.1088/0004-6256/139/5/1831
- ^ a b c d R. バーナム Jr. 著、斉田博 訳 『星百科大事典 改訂版』地人書館、1988年2月10日、972-975頁。ISBN 4-8052-0266-1。
- ^ a b c Duerbeck, Hilmar W. (1987), “A reference catalogue and atlas of galactic novae”, Space Science Review 45 (1-2): 1-212, Bibcode: 1987SSRv...45....1D, doi:10.1007/BF00187826
- ^ 神田茂「艫座新星に就いて」(PDF)『天文月報』第36巻第1号、1-5頁、1943年1月 。
- ^ 山本一淸「報告せざる觀測は價値乏し、等々」(PDF)『天界』第23巻第8号、241-243頁、1943年8月25日 。
- ^ a b c Orio, M.; et al. (2009-01), “New X-Ray Observations of the Old Nova CP Puppis and of the More Recent Nova V351 Puppis”, Astrophysical Journal 690 (2): 1753-1763, arXiv:0809.3992, Bibcode: 2009ApJ...690.1753O, doi:10.1088/0004-637X/690/2/1753
- ^ William, Robert E. (1982-10-01), “Spectroscopic analysis of the extended shells around the novae CP Puppis and T Pyxidis”, Astrophysical Journal 261: 173-182, Bibcode: 1982ApJ...261..170W, doi:10.1086/160328
- ^ Mason, E.; et al. (2013-11), “On the nature of CP Pup”, Monthly Notices of the Royal Astronomical Society 436 (1): 212-221, Bibcode: 2013MNRAS.436..212M, doi:10.1093/mnras/stt1565
- ^ “Introduction to Cataclysmic Variables (CVs)”. High Energy Astrophysics Science Archive Research Center. NASA GSFC. 2019年9月13日閲覧。
- ^ a b c O'Donoghue, D.; et al. (1989-09-01), “On the nature of the old nova CP Puppis”, Monthly Notices of the Royal Astronomical Society 240: 41-61, Bibcode: 1989MNRAS.240...41O, doi:10.1093/mnras/240.1.41
- ^ Cropper, M. (1986-09-15), “Polarization observations of DQ HER stars and other cataclysmic variables”, Monthly Notices of the Royal Astronomical Society 222: 225-233, Bibcode: 1986MNRAS.222..225C, doi:10.1093/mnras/222.2.225
- ^ Warner, B. (1985-11-01), “CP Puppis and V1500 Cygni”, Monthly Notices of the Royal Astronomical Society 217: 1P-5P, Bibcode: 1985MNRAS.217P...1W, doi:10.1093/mnras/217.1.1P
- ^ Bianchini, A.; Friedjung, M.; Sabbadin, F. (1985-01), “Probable Detection of a Very Short Orbital Period for the Old Classical Nova CP Puppis (1942)”, Information Bulletin on Variable Stars 2650: 1, Bibcode: 1985IBVS.2650....1B
- ^ a b White, James C., II; Honeycutt, R. K.; Horne, Keith (1993-07), “CP Puppis - No ordinary old nova”, Astrophysical Journal 412 (1): 278-287, Bibcode: 1993ApJ...412..278W, doi:10.1086/172918
- ^ Cropper, Mark (1990-12), “The Polars”, Space Science Reviews 54: 195-295, Bibcode: 1990SSRv...54..195C, doi:10.1007/BF00177799
- ^ Balman, Solen; Orio, Marina; Ogelman, Hakki (1995-08), “ROSAT Observation of the Old Classical Nova CP Puppis”, Astrophysical Journal Letters 449: L47-L50, Bibcode: 1995ApJ...449L..47B, doi:10.1086/309628
- ^ a b c Bianchini, A.; et al. (2012-03), “The old nova CP Puppis: a carbon nova and asynchronous polar?”, Astronomy & Astrophysics 539: A94, Bibcode: 2012A&A...539A..94B, doi:10.1051/0004-6361/201117251
- ^ Szkody, Paula; Feinswog, Laurie (1988-11-01), “Infrared light curves of three novae and three dwarf novae at quiescence”, Astrophysical Journal 334: 422-429, Bibcode: 1988ApJ...334..422S, doi:10.1086/166846
- ^ Prialnik, Dina; Kovetz, Attay (1995-06), “An extended grid of multicycle nova evolution models”, Astrophysical Journal 445 (2): 789-810, Bibcode: 1995ApJ...445..789P, doi:10.1086/175741
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