Pulsation-driven superwinds and internal evolution of intermediate-mass stars

Details Pulsation-driven superwinds and internal evolution of intermediate-mass stars Pulsation-driven superwinds and internal evolution of intermediate-mass stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..292..241b&link_type=abstract

Interplay of Periodic, Cyclic and Stochastic Variability in Selected Areas of the H-R Diagram. Edited by C. Sterken, ASP Conf. S

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Pulsationally excited winds are usually invoked to explain the high
mass-loss rates from AGB stars. We present semi-empirical formulae to
model the mass-loss rates in different parts of the HRD and then
apply these to study the effect of superwinds on the internal structure
of the stars and on the evolution towards the white-dwarf phase.

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