Type Ia supernova progenitors, lifetime, and cosmic supernova rate

被引：0
|
作者：
Kobayashi, C [1 ]
Nomoto, KI [1 ]
机构：
[1] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源：
FROM TWILIGHT TO HIGHLIGHT: THE PHYSICS OF SUPERNOVAE | 2003年
关键词：
D O I：
10.1007/10828549_51
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We make a comparison of the lifetime distribution derived from several models of Type Ia Supernovae (SNe Ia) and evaluate the SN Ia models from the observational constraints. Our SN Ia model, which is based on the single degenerate scenario and includes the metallicity effect, gives better reproduction of the [O/Fe]-(Fe/H) relation in the solar neighborhood if compared to, e.g., Matteucci & Recchi (2001). We also provide predictions of the cosmic supernova rate history.
引用
收藏
页码：379 / 383
页数：5
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