摘要
在转动双星系统非对称旋转椭球体模型下提出了各向异性的星风损失和角动量损失,数值模拟分析了转动双星系统的星风损失和角动量损失的分布,以及转动双星系统的演化,并给出相关结论。
Anisotropic mass and angular momentum losses via stellar wind are presented.The model is based on a non-symmetric rotational ellipsoid in the rotational binary system.Furthermore,the distributions of the mass and angular momentum losses and the evolution of the rotational binary system are simulated and analyzed.Then the corresponding conclusions are drawn.
出处
《山东大学学报（理学版）》
CAS
CSCD
北大核心
2010年第3期23-28,共6页
Journal of Shandong University(Natural Science)
基金
贵州省优秀科技教育人才省长专项资金项目(黔省专合字(2007)10号)
关键词
转动双星系统
星风损失
角动量损失
演化
the rotational binary system
mass loss due to stellar wind
angular momentum loss
evolution
