中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star

文献类型:期刊论文

作者YanKe Tang1; ShaoLan Bi2; Ning Gai1; HuaYin Xu1
刊名中国天文和天体物理学报:英文版
出版日期2008
卷号8.0期号:004页码:421
关键词星体 自转 磁场 频率 观测设备 观测方法
ISSN号1009-9271
英文摘要Taking into consideration the effects of rotation and interior magnetic field during the lifetime of the star, we reconstruct the model of α Cen B to satisfy the latest nonasteroseismic and asteroseismic observational constraints. We find that the effects can induce a change of about 0.3 μHz in the large frequency spacings and can speed up the star's evolution. The model of a Cen B has thereby been improved.
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/56822]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.北京师范大学
推荐引用方式
GB/T 7714
YanKe Tang,ShaoLan Bi,Ning Gai,等. Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star[J]. 中国天文和天体物理学报:英文版,2008,8.0(004):421.
APA YanKe Tang,ShaoLan Bi,Ning Gai,&HuaYin Xu.(2008).Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star.中国天文和天体物理学报:英文版,8.0(004),421.
MLA YanKe Tang,et al."Asteroseismic Analysis of α Cen B: Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star".中国天文和天体物理学报:英文版 8.0.004(2008):421.

入库方式: OAI收割

来源:国家天文台

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