Reference : Instability strip for pre-main-sequence stars

	Document type :	Scientific journals : Article
	Discipline(s) :	Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
	To cite this reference:	http://hdl.handle.net/2268/75453

Title :	Instability strip for pre-main-sequence stars
Language :	English
Author, co-author :	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) >]
Publication date :	1-Jan-2006
Journal title :	Communications in Asteroseismology
Volume :	147
Pages :	69-71
Audience :	International
Abstract :	[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.
Permalink :	http://hdl.handle.net/2268/75453
DOI :	10.1553/cia147s69
Other URL :	http://adsabs.harvard.edu/abs/2006CoAst.147...69G

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