Grid of solar-metallicity wind models (Mattsson+, 2010)

Astronomy and Astrophysics – Astronomy

Scientific paper

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Models: Atmosphere, Stars: Carbon, Stars: Giant, Mass Loss

Scientific paper

The file online.dat contains all the data presented in the paper. The table include input parameters and the resulting mean mass loss rate, mean velocity at the outer boundary and mean degree of dust condensation at the outer boundary. The dust-to-gas mass ratio is calculated as described in Hofner & Dorfi (1997A&A...319..648H).
A FORTRAN code representing a parametric mass-loss prescription for, e.g., stellar evolution modelling, is available at
http://coolstars.astro.uu.se
where also future updates will be posted.
(1 data file).

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