中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The effect of gravity darkening on spectral lines in a rotating star

文献类型:期刊论文

作者Dan HG(单红光)
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期2000-01
卷号24期号:1页码:81-87
关键词star rotation gravity darkening
ISSN号0275-1062
产权排序第一完成单位
通讯作者Shan, HG
英文摘要For rapidly rotating stars, the effect of gravity darkening on the equivalent width (EW) of spectral lines is very small, even when the rotation velocity is close to the critical velocity. But the effect on the full-width at half-maximum (FWHM) is relatively strong. At omega approximate to 0.99, the variation is 8%. For main-sequence stars in the range of spectral type B0 to B9, the variation of FWHM is almost independent of the spectral type when the rotation is small (omega < 0.8); for rapidly rotators (omega approximate to 0.99), the percentage variation of FWHM decreases with advancing spectral subclass.
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://www.sciencedirect.com/science/article/pii/S0275106200000308
语种英语
WOS记录号WOS:000085908600013
源URL[http://ir.ynao.ac.cn/handle/114a53/5153]  
专题云南天文台_恒星物理研究组
作者单位Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 ROC
推荐引用方式
GB/T 7714
Dan HG. The effect of gravity darkening on spectral lines in a rotating star[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2000,24(1):81-87.
APA Dan HG.(2000).The effect of gravity darkening on spectral lines in a rotating star.CHINESE ASTRONOMY AND ASTROPHYSICS,24(1),81-87.
MLA Dan HG."The effect of gravity darkening on spectral lines in a rotating star".CHINESE ASTRONOMY AND ASTROPHYSICS 24.1(2000):81-87.

入库方式: OAI收割

来源:云南天文台

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