Progenitors of type Ia supernovae

被引：74

作者：

Maeda, Keiichi ^{[1
]}

Terada, Yukikatsu ^{[2
]}

机构：

[1] Kyoto Univ, Dept Astron, Sakyo Ku, Kitashirakawa Oiwake Cho, Kyoto 6068502, Japan

[2] Saitama Univ, Grad Sch Sci & Engn, 255 Shimo Ohkubo, Sakura, Saitama 3388570, Japan

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2016年 / 25卷 / 10期

关键词：

Supernovae; binary stars; white dwarfs; DELAYED-DETONATION MODELS; GAMMA-RAY EMISSION; ACCRETION-INDUCED COLLAPSE; CHANDRASEKHAR MASS MODELS; WHITE-DWARF MODELS; LATE-TIME SPECTRA; SN; 2014J; SODIUM-ABSORPTION; LIGHT CURVES; CIRCUMSTELLAR MATERIAL;

D O I：

10.1142/S021827181630024X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Natures of progenitors of type Ia Supernovae (SNe Ia) have not yet been clarified. There has been long and intensive discussion on whether the so-called single degenerate (SD) scenario or the double degenerate (DD) scenario, or anything else, could explain a major population of SNe Ia, but the conclusion has not yet been reached. With rapidly increasing observational data and new theoretical ideas, the field of studying the SN Ia progenitors has been quickly developing, and various new insights have been obtained in recent years. This paper aims at providing a summary of the current situation regarding the SN Ia progenitors, both in theory and observations. It seems difficult to explain the emerging diversity seen in observations of SNe Ia by a single population, and we emphasize that it is important to clarify links between different progenitor scenarios and different sub-classes of SNe Ia.

引用

页数：22

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