Paper:	Mass-Loss and Multicomponent Flow from Central Stars of Planetary Nebulae
Volume:	334, 14th European Workshop on White Dwarfs
Page:	337
Authors:	Krticka, J.; Kubat, J.
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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.044 seconds