Signature of main sequence internal structure in post-main sequence stars

Bibcode
2009CoAst.158..239D
Dupret, M.-A.; Godart, M.; Noels, A.; Lebreton, Y.
Referencia bibliográfica

"Communications in Asteroseismology, Vol.158, p. 239 Proceedings of "38th Liege International Astrophysical Colloquium: Evolution and Pulsation of Massive Stars on the Main Sequence and Close to it", held on July 7-11 2008, edited by Arlette Noels, Conny Aerts, Josefina Montalban, Andrea Miglio and Maryline Briquet."

Fecha de publicación:
7
2009
Número de autores
4
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
5
Descripción
Post Main Sequence (post MS) stars keep a trace of their past main sequence history. Typically, the presence or not of an Intermediate Convective Zone (ICZ) above the H-burning shell of massive stars critically depends on the details of the Main Sequence (MS) phase modeling (convection criterion, mass loss,~...). We show here how the excitation of g-modes in blue supergiant stars is closely related to this ICZ, allowing to constrain different associated physical processes.
Tipo
Sin árbitro

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