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Non-adiabatic seismic study of the triple system DG Leo
Grigahcène, A.; Suárez, J. C.; Dupret, Marc-Antoine et al.
2005In Tidal Evolution and Oscillations in Binary Stars
 

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Abstract :
[en] The interest in studying multiple systems comes from the fact that they give a good number of constraints on their components. From the multiplicity we have constraints on mass and age. Moreover, if one or more components of the system show oscillating properties as the DG Leo triple system, additional constraints provided by seismology can be obtained once the modes are identified. In this work, we consider an equilibrium model of the DG Leo system constrained by its multiplicity properties, we attempt to check our new Time Depending Convection treatment on the modes identification of the DG Leo system.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Grigahcène, A.
Suárez, J. C.
Dupret, Marc-Antoine ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique
Garrido, R.
Language :
English
Title :
Non-adiabatic seismic study of the triple system DG Leo
Publication date :
01 November 2005
Audience :
International
Main work title :
Tidal Evolution and Oscillations in Binary Stars
Pages :
242
Commentary :
333
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since 11 November 2010

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