Mass-loss from Red Giants

Details Mass-loss from Red Giants Mass-loss from Red Giants

2008-03-07

arxiv.org/abs/0803.1170v2

Astronomy and Astrophysics

Astrophysics

Revised version of review submitted to the RS Oph meeting, Keele 2007

Scientific paper

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.

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