Mass loss, meridional circulation and turbulence in contemporary stellar evolution models

Details Mass loss, meridional circulation and turbulence in contemporary stellar evolution models Mass loss, meridional circulation and turbulence in contemporary stellar evolution models

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224...59t&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Physics

1

Turbulence, Hydrodynamics, Stars: Abundances, Stars: Evolution, Stars: Chemically Peculiar, Hertzsprung-Russell Diagram, Stars: Interiors, Stars: Mass Loss, Stars: Rotation.

Scientific paper

In this review, I will briefly discuss the hypotheses made in the treatment of modern rotating stellar models and review the expected efficiency of mixing along the HR diagram. The role of mixing in the localization of abundance anomalies will also be discussed. Finally, I will show how mass loss and gravitational settling of helium may influence the evolution of rotating stars, and how A stars can play a unique role in constraining our models.

Affiliated with

Also associated with

No associations

Rating

Mass loss, meridional circulation and turbulence in contemporary stellar evolution 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, meridional circulation and turbulence in contemporary stellar evolution models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mass loss, meridional circulation and turbulence in contemporary stellar evolution models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1083047