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Asteroseismic Analysis ofαCen B:Preliminary Tests of Effects of Rotation and Interior Magnetic Field in the Solar-like Star

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【Author】 Yan-Ke Tang~(1,3) Shao-Lan Bi~(2,1) Ning Gai~(1,3) Hua-Yin Xu~1 1 National Astronomical Observatories / Yunnan Observatory,Chinese Academy of Sciences,Kunming 650011,China; 2 Department of Astronomy Beijing Normal University,Beijing 100875,China 3 Graduate School of Chinese Academy of Sciences,Beijing 100049,China

【摘要】 <正>Taking into consideration the effects of rotation and interior magnetic field dur- ing the lifetime of the star,we reconstruct the model ofαCen B to satisfy the latest non- asteroseismic and asteroseismic observational constraints.We find that the effects can induce a change of about 0.3μHz in the large frequency spacings and can speed up the star’s evolu- tion.The model ofαCen B has thereby been improved.

【Abstract】 Taking into consideration the effects of rotation and interior magnetic field dur- ing the lifetime of the star,we reconstruct the model ofαCen B to satisfy the latest non- asteroseismic and asteroseismic observational constraints.We find that the effects can induce a change of about 0.3μHz in the large frequency spacings and can speed up the star’s evolu- tion.The model ofαCen B has thereby been improved.

【基金】 The Ministry of Science and Technology of the People’s Republic of China through Grant 2007CB815406;the NSFC through Grants 10173021,10433030,10773003 and 10778601
  • 【文献出处】 Chinese Journal of Astronomy and Astrophysics ,中国天文和天体物理学报(英文版) , 编辑部邮箱 ,2008年04期
  • 【分类号】P144.7
  • 【下载频次】4
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