Mass Loss Characteristics of Dust Forming Long-Period Variable Stars

Details Mass Loss Characteristics of Dust Forming Long-Period Variable Stars Mass Loss Characteristics of Dust Forming Long-Period Variable Stars

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001assl..265...93w&link_type=abstract

Post-AGB Objects as a Phase of Stellar Evolution, Proceedings of the Toruń Workshop held July 5-7, 2000. Edited by R. Szczerba a

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

We present results obtained from a grid of model calculations for dust forming circumstellar shells around carbon-rich long-period variable stars. These models consistently treat the time-dependent hydrodynamics, chemistry, dust formation and the radiative transfer problem. We show that variations of the mass loss rates observed on different time scales are well reproduced by our models.

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