Modelling convection and semiconvection in massive stars

Details Modelling convection and semiconvection in massive stars Modelling convection and semiconvection in massive stars

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.158...79c&link_type=abstract

"Communications in Asteroseismology, Vol.158, p. 79 Proceedings of "38th Liege International Astrophysical Colloquium: Evolutio

Astronomy and Astrophysics

Astrophysics

Scientific paper

Massive stars the ideal laboratory to investigate three important physical phenomena: mass loss by stellar wind, convective instability and associated mixing, rotation, and their interplay. In this note, we will focus on the convective instability, summarizing the results obtained over the past three decades and highlighting some points that are still controversial.

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