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激变双星的角动量损失机制和演化
毕少兰
1994
Source Publication天体物理学报
ISSN0253-2379
Volume014Issue:002Pages:151
Abstract本文详细研究了激变双星系统的演化,发现磁制动机制导致的角动量损失要求星风的量级为10^-11—10^-12M⊙yr^-1,这比太阳风强10^2-10^3倍,表明磁星风机制失效。作者认为驱动双星系统演化的角动量损失是由来自致密星的吸积盘外边缘的物质溢出的惯性离心力所致。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/41122
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
毕少兰. 激变双星的角动量损失机制和演化[J]. 天体物理学报,1994,014(002):151.
APA 毕少兰.(1994).激变双星的角动量损失机制和演化.天体物理学报,014(002),151.
MLA 毕少兰."激变双星的角动量损失机制和演化".天体物理学报 014.002(1994):151.
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