Modelling massive stars with mass loss

Details Modelling massive stars with mass loss Modelling massive stars with mass loss

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.158...87e&link_type=abstract

"Communications in Asteroseismology, Vol.158, p. 87 Proceedings of "38th Liege International Astrophysical Colloquium: Evolutio

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Mass loss plays a major role in the evolution of massive stars. Its effects on the modelling of massive stars (in particular internal structure, evolutionary tracks in the HR diagram, lifetimes, and surface abundances) will first be presented in detail. The modelling of Wolf-Rayet stars will then be examined. The interaction between mass loss and rotation, as well as between mass loss and pulsation, will finally be briefly discussed.

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