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.

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