Mass loss in 2D Rotating Stellar Models

Details Mass loss in 2D Rotating Stellar Models Mass loss in 2D Rotating Stellar Models

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011bsrsl..80..165l&link_type=abstract

Société Royale des Sciences de Liège, Bulletin, vol. 80, p. 165-169 (Proceedings of the 39th Liège Astrophysical Colloquium, hel

Astronomy and Astrophysics

Astrophysics

Scientific paper

Radiatively driven mass loss is an important factor in the evolution of massive stars. The mass-loss rates depend on a number of stellar parameters, including the effective temperature and luminosity. Massive stars are also often rapidly rotating, which affects their structure and evolution. In sufficiently rapidly rotating stars, both the effective temperature and radius vary significantly as a function of latitude, and hence mass loss rates can vary appreciably between the poles and the equator. In this work, we discuss the addition of mass loss to a 2D stellar evolution code (ROTORC) and compare evolution sequences with and without mass loss.

Affiliated with

Also associated with

No associations

Rating

Mass loss in 2D Rotating Stellar Models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mass loss in 2D Rotating Stellar Models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass loss in 2D Rotating Stellar Models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1588255