Modelling of the spectra and atmospheres of evolved stars

The method and results of the computation of the model atmospheres and spectral energy distributions of chemically peculiar stars, are discussed. The models are computed with a special consideration of the particular problems encountered when computing model atmospheres for M and C-giants, and of hy...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2006-06
Main Author: Pavlenko, Yakiv V
Format: Article
Language:English
Subjects:
Atmospheric models
Computation
Globular clusters
Organic chemistry
Peculiar stars
Stars
Stellar atmospheres
Stellar evolution
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:The method and results of the computation of the model atmospheres and spectral energy distributions of chemically peculiar stars, are discussed. The models are computed with a special consideration of the particular problems encountered when computing model atmospheres for M and C-giants, and of hydrogen deficient stars. We present some computed model atmospheres for Sakurai's object, giants of globular clusters, and C-giants.
ISSN:2331-8422