ASPCS
 
Back to Volume
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.
eAccess Cost: $9.00
Back to Volume