The Structure of Winds in AGB Stars

Details The Structure of Winds in AGB Stars The Structure of Winds in AGB Stars

2002-07-23

arxiv.org/abs/astro-ph/0207513v1

Astronomy and Astrophysics

Astrophysics

To appear in proc. of "Workshop on Mass-Losing Pulsating Stars and their Circumstellar Matter", Sendai, Japan (May 2002)

Scientific paper

Most dusty winds are described by a set of similarity functions of a single
independent variable that can be chosen as the overall optical depth at visual.
The self-similarity implies general scaling relations among the system
parameters, in agreement with observations. Dust drift through the gas has a
major impact on the structure of most winds.

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