Mass-loss and multicomponent flow from central stars of planetary nebulae
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0410303,
title = {Mass-loss and multicomponent flow from central stars of planetary nebulae},
author = {Jiri Krticka and Jiri Kubat},
journal= {arXiv preprint arXiv:astro-ph/0410303},
year = {2007}
}
Comments
4 pages; to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler