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

2002/08/09 by K. Werner, Werner, K., J. L. Deetjen +7
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0208199

To 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

arxiv created 2002/08/09 · openalex publication_date 2002/08/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We 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.

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