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

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dc.creatorKrticka, Jiri
dc.creatorKubat, Jiri
dc.date2004-10-12
dc.date.accessioned2026-07-07T02:15:04Z
dc.date.available2026-07-07T02:15:04Z
dc.descriptionWe 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.
dc.description4 pages; to appear in 14th European Workshop on White Dwarfs, ASP Conference Series, eds. D. Koester, S. Moehler
dc.identifierhttps://arxiv.org/abs/astro-ph/0410303
dc.identifierhttp://arxiv.org/abs/astro-ph/0410303
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8358
dc.subjectAstrophysics
dc.titleMass-loss and multicomponent flow from central stars of planetary nebulae
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