Seismic modelling of OB stars

[en] A review of the ability of asteroseismology to probe the internal physics of OB stars is presented. The main constraints that can be obtained from the frequency spectrum in p- and g-modes pulsators are discussed. Next, we consider energetic aspects of the pulsations in OB stars and show how such study also allows to constrain their internal physics. The cases of p-mixed modes (β Cep stars), g-modes (SPB stars), strange modes and stochastically excited modes are considered.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Dupret, Marc-Antoine ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie

Godart, Mélanie ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie

Belkacem, Kevin ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie

Noels-Grötsch, Arlette ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie

Language :

English

Title :

Seismic modelling of OB stars

Publication date :

01 July 2011

Journal title :

Proceedings of the International Astronomical Union

ISSN :

1743-9213

eISSN :

1743-9221

Publisher :

Cambridge University Press, Cambridge, United Kingdom

Volume :

272

Pages :

457-467

Additional URL :

http://adsabs.harvard.edu/abs/2011IAUS..272..457D

Available on ORBi :

since 10 January 2012

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