Rotation of the accreting white dwarfs and diversity of Type Ia supernovae

被引：2
|
作者：
Uenishi, T
Nomoto, K
Hachisu, I
机构：
[1] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[2] Univ Tokyo, Coll Arts & Sci, Dept Earth Sci & Astron, Meguro Ku, Tokyo 1538902, Japan
来源：
NUCLEAR PHYSICS A | 2003年 / 718卷
关键词：
D O I：
10.1016/S0375-9474(03)00905-9
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
We consider rotation of progenitor white dwarfs for a possible source of the diversity of Type Ia supernovae (SNe Ia). Hydrostatic structure of rotating white dwarfs with different masses are calculated. Evolutionary sequences of white dwarfs are explored and the effect of "supercritical" rotation in binary system is examined. Possible effects of rotation to cause diversity of SNe Ia are discussed.
引用
收藏
页码：623C / 625C
页数：3
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