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

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

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.158..239d&link_type=abstract

"Communications in Asteroseismology, Vol.158, p. 239 Proceedings of "38th Liege International Astrophysical Colloquium: Evoluti

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

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.

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