Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars

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dc.creatorWerner, K.
dc.creatorDeetjen, J. L.
dc.creatorDreizler, S.
dc.creatorNagel, T.
dc.creatorRauch, T.
dc.date2002-08-09
dc.date.accessioned2026-07-07T02:04:38Z
dc.date.available2026-07-07T02:04:38Z
dc.descriptionWe describe our NLTE codes which allow the computation of synthetic spectra of hot stars and accretion disks. They can be combined to compute ionizing fluxes from the hot component in symbiotic stars.
dc.descriptionTo be published in: Symbiotic stars probing stellar evolution, R.L.M. Corradi, J. Mikolajewska, and T.J. Mahoney, eds., ASP Conference Series, 4 pages, no figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0208199
dc.identifierhttp://arxiv.org/abs/astro-ph/0208199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4835
dc.subjectAstrophysics
dc.titleStellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars
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