Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars
Astrophysics
2007-05-23 v1
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.
Cite
@article{arxiv.astro-ph/0208199,
title = {Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars},
author = {K. Werner and J. L. Deetjen and S. Dreizler and T. Nagel and T. Rauch},
journal= {arXiv preprint arXiv:astro-ph/0208199},
year = {2007}
}
Comments
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