asteroseismicanalysisofcenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar
文献类型：期刊论文
| 作者 | YanKe Tang1; ShaoLan Bi2; Ning Gai1; HuaYin Xu1 |
| 刊名 | chinesejournalofastronomyandastrophysics
 |
| 出版日期 | 2008 |
| 卷号 | 008期号:004页码:421 |
| 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/114a11/53740]  |
| 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,et al. asteroseismicanalysisofcenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar[J]. chinesejournalofastronomyandastrophysics,2008,008(004):421. |
| APA | YanKe Tang,ShaoLan Bi,Ning Gai,&HuaYin Xu.(2008).asteroseismicanalysisofcenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar.chinesejournalofastronomyandastrophysics,008(004),421. |
| MLA | YanKe Tang,et al."asteroseismicanalysisofcenbpreliminarytestsofeffectsofrotationandinteriormagneticfieldinthesolarlikestar".chinesejournalofastronomyandastrophysics 008.004(2008):421. |
入库方式： OAI收割
来源：国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。