The Evolution of Cataclysmic Variables
Li LF(李立芳)1,2; Zhang FH(张奉辉)1,2; Han ZW(韩占文)1,2
2013-02
会议名称290th IAU Symposium - Feeding Compact Objects: Accretion on All Scales
会议日期2012-08-20
会议地点Beijing, China
关键词Stars: cataclysmic variables stars: evolution stars: magnetic fiels stars: mass-loss
卷号290
页码253-254
英文摘要Using Eggletons code the evolution of cataclysmic variables (CVs) is investigated. CVs might suffer the loss of mass and angular momentum during their evolution, we present the models of CVs with mass loss and angular momentum loss (AML) due to gravitation wave radiation (GR) and/or magnetic braking (MB). It is found that the loss of mass and angular momentum has significant influence on the evolution of CVs, and that the change of the star structure or their atmosphere properties is a possible mechanism which underlies a sudden change in the rate of AML owing to MB.
收录类别其他
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会议网址http://adsabs.harvard.edu/abs/2013IAUS..290..253L
会议录Proceedings of the International Astronomical Union, IAU Symposium - Feeding Compact Objects: Accretion on All Scales
学科主题Astronomy & Astrophysics
语种英语
内容类型会议论文
源URL[http://ir.ynao.ac.cn/handle/114a53/261]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.National Astronomical Observatories/Yunnan Observatory, CAS, P.O. Box 110, Kunming, Yunnan Province, 650011, P.R. China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, P.O. Box 110, Kunming, Yunnan Province, 650011, P.R. China
推荐引用方式
GB/T 7714
Li LF,Zhang FH,Han ZW. The Evolution of Cataclysmic Variables[C]. 见:290th IAU Symposium - Feeding Compact Objects: Accretion on All Scales. Beijing, China. 2012-08-20.http://adsabs.harvard.edu/abs/2013IAUS..290..253L.
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