Massive Star Evolution with Mass Loss and Rotation

Details Massive Star Evolution with Mass Loss and Rotation Massive Star Evolution with Mass Loss and Rotation

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33...38m&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

5

Stars: Evolution, Stars: Mass Loss, Stars: Rotation, Stars: Wolf-Rayet

Scientific paper

Stellar rotation influences the tracks, the lifetimes, the mass determinations, the chemical composition of massive stars, as well as the formation of red supergiants and WR stars. The anisotropic mass loss rates of massive rotating stars is an essential feature for accounting LBV nebulae. It also leads to WO stars with little or no He left, keeping at the same time a high enough rotation to produce a possible GRB precursor.

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