NAOC Open IR
自转对恒星物理量的影响
谭徽松; 潘开科
1996
Source Publication云南天文台台刊
ISSN1001-7526
Volume000Issue:002Pages:1
Abstract自转本身是恒星的基本物理量之一,同时影响恒星的其它许多物物量,包括对情理星半径、形状和体积的影响。对光度,色指数、谱线轮廓,先进值宽度,偏振度等观测量的影响;对引力加速度,元素丰度的影响;对恒星内部结构,如中心压力,温度,密度的影响。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47046
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
谭徽松,潘开科. 自转对恒星物理量的影响[J]. 云南天文台台刊,1996,000(002):1.
APA 谭徽松,&潘开科.(1996).自转对恒星物理量的影响.云南天文台台刊,000(002),1.
MLA 谭徽松,et al."自转对恒星物理量的影响".云南天文台台刊 000.002(1996):1.
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