Reference : Instability strip for pre-main-sequence stars
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/75453
Instability strip for pre-main-sequence stars
English
Grigahcene, A. [> > > >]
Dupret, Marc-Antoine [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique >]
Garrido, R. [> > > >]
Gabriel, Maurice [> > Département d'astrophys., géophysique et océanographie (AGO) >]
Scuflaire, Richard [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA) >]
1-Jan-2006
Communications in Asteroseismology
147
69-71
Yes
International
[en] We apply the Time Dependent Convection (TDC) treatment presented in Grigahcene et al. (2005) to the study of Pre-main sequence pulsating stars. The stabilization of the p-modes at the red edge of the Instability Strip (IS) is obtained by our models. The theoretical IS obtained with Mixing Length (ML) parameter alpha=1.8 is compared to observations and a good agreement is obtained.
http://hdl.handle.net/2268/75453
10.1553/cia147s69
http://adsabs.harvard.edu/abs/2006CoAst.147...69G

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