pith. sign in

arxiv: astro-ph/0208199 · v1 · submitted 2002-08-09 · 🌌 astro-ph

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

classification 🌌 astro-ph
keywords starsaccretioncomponentsymbioticallowatmospherecodescombined
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.