Reference : Non-adiabatic seismic study of the triple system DG Leo
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/75491
Non-adiabatic seismic study of the triple system DG Leo
English
Grigahcène, A. [> > > >]
Suárez, J. C. [> > > >]
Dupret, Marc-Antoine [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique >]
Garrido, R. [> > > >]
1-Nov-2005
Tidal Evolution and Oscillations in Binary Stars
242
No
No
International
[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.
http://hdl.handle.net/2268/75491
http://adsabs.harvard.edu/abs/2005ASPC..333..242G
333

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Open access
333-0242.pdfPublisher postprint202.76 kBView/Open

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.