NAOC Open IR
吸积盘边缘的质量和角动量损失与激变双星的演化
余君岳1; 黄润乾2
1996
Source Publication天体物理学报
ISSN0253-2379
Volume016Issue:001Pages:41
Abstract本文给出了计算吸积盘边缘物质和角动量损失,以及它们对激变双星演化影响的理论模型。计算结果表明,紫外天文卫星(IUE)观测到的高速物质流是来源于吸积盘边缘,吸积盘边缘的角动量损失可以成为周期大于3小时的激变双星演化的物理机制。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/51505
Collection中国科学院国家天文台
Affiliation1.香港城市大学
2.中国科学院国家天文台
Recommended Citation
GB/T 7714
余君岳,黄润乾. 吸积盘边缘的质量和角动量损失与激变双星的演化[J]. 天体物理学报,1996,016(001):41.
APA 余君岳,&黄润乾.(1996).吸积盘边缘的质量和角动量损失与激变双星的演化.天体物理学报,016(001),41.
MLA 余君岳,et al."吸积盘边缘的质量和角动量损失与激变双星的演化".天体物理学报 016.001(1996):41.
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