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

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

2002-08-09

arxiv.org/abs/astro-ph/0208199v1

Astronomy and Astrophysics

Astrophysics

To be published in: Symbiotic stars probing stellar evolution, R.L.M. Corradi, J. Mikolajewska, and T.J. Mahoney, eds., ASP Co

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Atmosphere and Accretion Disk Models for the Hot Component in Symbiotic Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-665807