ORBi: Bouabid M*-P - Theoretical study of γ Doradus pulsations in pre-main sequence stars

Reference : Theoretical study of γ Doradus pulsations in 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/2268/81906

Title :	Theoretical study of γ Doradus pulsations in pre-main sequence stars
Language :	English
Author, co-author :	Bouabid, M-P [UMR 6525 H. Fizeau, UNS, CNRS, OCA, Campus Valrose, F-06108 Nice Cedex 2, France; Institut d'Astrophysique et de Géophysique de l'Université de Liège, Allée du 6 Août, 17 B-4000 Liège, Belgium]*
	Montalban Iglesias, Josefa [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie]
	Miglio, Andrea [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie]
	Dupret, Marc-Antoine [Institut d'Astrophysique et de Géophysique de l'Université de Liège, Allée du 6 Août, 17 B-4000 Liège, Belgium]
	Grigahcène, A. [Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal]
	Noels-Grötsch, Arlette [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Publication date :	2010
Journal title :	Astronomische Nachrichten
Publisher :	Wiley
Volume :	331
Pages :	1044
Audience :	International
ISSN :	0004-6337
e-ISSN :	1521-3994
City :	Berlin
Country :	Germany
Keywords :	[en] stars: oscillations ; stars: pre-main sequence
Abstract :	[en] The question of the existence of the pre-main sequence (PMS) γ Doradus (γ Dor) pulsators has been raised by observations of young clusters such as NGC 884 hosting γ Dor members. We have explored the properties of γ Dor-type pulsations with a grid of PMS models covering the mass range {1.2 < M_*/M_ȯ < 2.5} and we derive the theoretical instability strip (IS) for the PMS γ Dor pulsators. We explore the possibility of distinguishing between PMS and MS γ Dor by the behaviour of the period spacing of their high order gravity modes (g-modes).
Permalink :	http://hdl.handle.net/2268/81906
DOI :	10.1002/asna.201011453
Other URL :	http://adsabs.harvard.edu/abs/2010AN....331.1044B
Commentary :	http://de.arxiv.org/abs/1007.2746

File(s) associated to this reference

Fulltext file(s):

	File	Commentary	Version	Size	Access
Restricted access	1044_ftp.pdf		Publisher postprint	164.69 kB	Request copy

All documents in ORBi are protected by a user license.

Dspace v1.5