Progenitors of Type Ia Supernovae: Single Degenerate and Double Degenerates

被引：0

作者：

Nomoto, Ken'ichi ^{[1
]}

Kamiya, Yasuomi ^{[1
,2
]}

Nakasato, Naohito ^{[3
]}

Hachisu, Izumi ^{[4
]}

Kato, Mariko ^{[5
]}

机构：

[1] Univ Tokyo, Inst Phys & Math Universe, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778568, Japan

[2] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan

[3] Univ Aizu, Dept Comp Sci & Engn, Aizu Wakamatsu, Fukushima 9658580, Japan

[4] Univ Tokyo, Coll Arts & Sci, Dept Earth Sci & Astron, Meguro Ku, Tokyo 1538902, Japan

[5] Keio Univ, Dept Astron, Kouhoku Ku, Yokohama 2238521, Japan

来源：

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE | 2009年 / 1111卷

关键词：

supernova; white dwarf; binary; ACCRETING WHITE-DWARFS; ELECTRON-CAPTURE SUPERNOVAE; DELAY-TIME DISTRIBUTION; LIGHT-CURVE MODEL; CORONAE BOREALIS; EVOLUTION; MASS; STARS; BINARIES; CHANNEL;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We summarize some recent developments in theoretical studies on the progenitors of Type Ia supernovae (SNe Ia): (1) merging of double degenerates and associated off-center carbon ignition, (2) mass-stripping from the companion star by white dwarf winds, (3) the formation of circumstellar matter and the young population of SNe Ia, (4) delay time distribution in the single degenerate scenario, and (5) the origin of the transient heavy element absorption systems observed in novae.

引用

页码：267 / +

页数：3

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