Mass-loss and multicomponent flow from central stars of planetary nebulae

Details Mass-loss and multicomponent flow from central stars of planetary nebulae Mass-loss and multicomponent flow from central stars of planetary nebulae

2004-10-12

arxiv.org/abs/astro-ph/0410303v1

Astronomy and Astrophysics

Astrophysics

4 pages; to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler

Scientific paper

We calculate multicomponent radiatively driven stellar wind models suitable
for central stars of planetary nebulae. Some of these stellar winds may be
adequately modelled using one-component models, however for some of them
multicomponent models are necessary. We obtain a range of stellar parameters
for different types of mass-loss.

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