中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The non-conservative evolution of massive binary systems

文献类型:期刊论文

作者Huang RQ(黄润乾)1,2; TAAM, RE3
刊名ASTRONOMY & ASTROPHYSICS
出版日期1990-09
卷号236期号:1页码:107-116
关键词evolution of binaries - mass loss
ISSN号0004-6361
产权排序第一完成单位
通讯作者HUANG, RQ (reprint author), CHINESE CTR ADV SCI & TECHNOL, CTR ASTRON & ASTROPHYS, WORLD LAB, BEIJING, PEOPLES R CHINA.
英文摘要The evolution of a massive binary system consisting of a 40- and 25-solar mass star has been studied in the conservative and nonconservative approximation in mass transfer phases, Case A and Case B. Specific attention is focused on the differences between the evolutions when account is taken of the enhancement of a stellar wind associated with tidal effects and irradiation. For the form of the mass loss formula adopted, only tidal effects were found to be important. The effect is significant in Case A, but not in Case B. The relation between mass and angular momentum loss is discussed.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
收录类别SCI
原文出处http://adsabs.harvard.edu/abs/1990A%26A...236..107H
语种英语
WOS记录号WOS:A1990DW13600017
源URL[http://ir.ynao.ac.cn/handle/114a53/9369]  
专题云南天文台_恒星物理研究组
作者单位1.Center of Astronomy and Astrophysics, CCAST (World Laboratory), Beijing, People's Republic of China
2.Yunnan Observatory, Kunming, People's Republic of China
3.Northwestern University, Department of Physics and Astronomy, Evanston, Illinois, USA
推荐引用方式
GB/T 7714
Huang RQ,TAAM, RE. The non-conservative evolution of massive binary systems[J]. ASTRONOMY & ASTROPHYSICS,1990,236(1):107-116.
APA 黄润乾,&TAAM, RE.(1990).The non-conservative evolution of massive binary systems.ASTRONOMY & ASTROPHYSICS,236(1),107-116.
MLA 黄润乾,et al."The non-conservative evolution of massive binary systems".ASTRONOMY & ASTROPHYSICS 236.1(1990):107-116.

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来源:云南天文台

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