Effects of rotation on stellar evolution and asteroseismology of red giants
Solar and Stellar Astrophysics
2015-06-22 v1
Abstract
The impact of rotation on the properties of low-mass stars at different evolutionary stages is first described by discussing the properties of stellar models computed with shellular rotation. The observational constraints that are currently available to progress in our understanding of these dynamical processes are then presented, with a peculiar focus on asteroseismic measurements of red-giant stars.
Keywords
Cite
@article{arxiv.1409.2269,
title = {Effects of rotation on stellar evolution and asteroseismology of red giants},
author = {Patrick Eggenberger},
journal= {arXiv preprint arXiv:1409.2269},
year = {2015}
}
Comments
Proc. of the workshop "Asteroseismology of stellar populations in the Milky Way" (Sesto, 22-26 July 2013), Astrophysics and Space Science Proceedings, (eds. A. Miglio, L. Girardi, P. Eggenberger, J. Montalban)