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Fundamental properties and seismological analysis of three Kepler stars

Published online by Cambridge University Press:  18 July 2013

K. Liu  and
S. L. Bi
K. Liu
Affiliation:
Deparment of Astronomy, Beijing Normal University, Beijing 100875, China email: liukang@mail.bnu.edu
S. L. Bi
Affiliation:
Deparment of Astronomy, Beijing Normal University, Beijing 100875, China email: liukang@mail.bnu.edu
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Abstract

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The lithium abundance of KIC 11395018 and KIC 10920273 are not compatible with their age, which is deduced by asteroseismology. To explain this phenomenon, we investigate the possible evolutionary status and perform seismological analysis of the three stars KIC 11395018, KIC 10273246 and KIC 10920273. Using the Yale Rotating Stellar Evolution Code (YREC), we constructed a grid of evolutionary tracks with different input physics and rotation rates. In addition to the conventional observed properties, we added two observed constraints: lithium abundance and rotational period. As a result, the lithium abundance of our rotation models agrees well with the observation. Meanwhile, we obtained a set of more accurate stellar fundamental parameters than previous studies.

Keywords

stars: fundamental parametersstars: rotationstars: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 203 - 204
Copyright
Copyright © International Astronomical Union 2013 

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