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
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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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