Article (Scientific journals)
Instability strip for pre-main-sequence stars
Grigahcene, A.; Dupret, Marc-Antoine; Garrido, R. et al.
2006In Communications in Asteroseismology, 147, p. 69-71
Peer reviewed
 

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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.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Grigahcene, A.
Dupret, Marc-Antoine ;  Université de Liège - ULiège > 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 - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Evol. et stabilité des étoiles et des amas d'étoiles (ESEA)
Language :
English
Title :
Instability strip for pre-main-sequence stars
Publication date :
01 January 2006
Journal title :
Communications in Asteroseismology
ISSN :
1021-2043
eISSN :
2224-8374
Publisher :
Verlag der Österreichischen Akademie der Wissenschaften, Wien, Austria
Volume :
147
Pages :
69-71
Peer reviewed :
Peer reviewed
Available on ORBi :
since 10 November 2010

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