Mass-loss from Red Giants
Astrophysics
2008-03-13 v2
Abstract
Although much is known about the nature of winds from hot stars and giants and supergiants with spectral types earlier than K, there is still much to be learned regarding the mass-loss process in cool, late-type stars. We will review the current state of research, with particular reference to observations and modelling of mass-loss from giant stars in symbiotic systems.
Keywords
Cite
@article{arxiv.0803.1170,
title = {Mass-loss from Red Giants},
author = {Brian Espey and Cian Crowley},
journal= {arXiv preprint arXiv:0803.1170},
year = {2008}
}
Comments
Revised version of review submitted to the RS Oph meeting, Keele 2007