A test of an early-type contact binary model by comparing the relations obtained from theory with those from observations
文献类型:期刊论文
作者 | Song F(宋芬)1,2![]() ![]() |
刊名 | SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
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出版日期 | 2012-02 |
卷号 | 55期号:2页码:320-328 |
关键词 | binaries: eclipsing stars: evolution stars: fundamental parameters stars: rotation |
ISSN号 | 1674-7348 |
产权排序 | 第二完成单位 |
通讯作者 | Song, F (reprint author), Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China. |
英文摘要 | Contact binary systems, including massive, middle-mass and low-mass systems, have been observed. It is necessary to construct the evolutionary model for contact binary systems with all different masses. The model introduced by Huang, Song and Bi indicates some special and unique understandings of the physical processes occurring in the contact binaries. It is necessary to test whether this model can be applied to the early-type contact binaries. The best way to test a theoretical model is to know whether this model can explain the observational phenomena of such binaries. For this aim, a comparison is performed for the relations of mass-luminosity, mass-radius, and the distribution in the HR diagram obtained from the model introduced by Huang et al. and those from the astronomical observations. A good result is obtained by the comparison. This means the model can be used in calculating the evolution of early-type contact binaries, and can explain the observational phenomena of such binaries. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Physics |
分类号 | P153 |
类目[WOS] | Physics, Multidisciplinary |
研究领域[WOS] | Physics |
关键词[WOS] | URSAE MAJORIS SYSTEMS ; OVERCONTACT BINARIES ; MARGINAL CONTACT ; EVOLUTION ; STARS ; PERIOD ; STABILITY ; CENTAURI ; CYGNI |
收录类别 | SCI ; EI |
原文出处 | http://link.springer.com/article/10.1007%2Fs11433-011-4615-3 |
语种 | 英语 |
WOS记录号 | WOS:000299295500019 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5226] ![]() |
专题 | 云南天文台_恒星物理研究组 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.Department of Astronomy, Beijing Normal University, Beijing, 100875, China 2.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, China 3.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650011, China |
推荐引用方式 GB/T 7714 | Song F,Huang RQ. A test of an early-type contact binary model by comparing the relations obtained from theory with those from observations[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2012,55(2):320-328. |
APA | Song F,&Huang RQ.(2012).A test of an early-type contact binary model by comparing the relations obtained from theory with those from observations.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,55(2),320-328. |
MLA | Song F,et al."A test of an early-type contact binary model by comparing the relations obtained from theory with those from observations".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 55.2(2012):320-328. |
入库方式: OAI收割
来源:云南天文台
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