Basic concepts of the stellar atmospheres theory are briefly outlined. After discussing essential assumptions, approximations, and basic structural equations describing a stellar atmospheres, emphasis is given to describing efficient numerical methods developed to deal with the stellar atmosphere problem, namely the method of complete linearization and its recent variants, and the whole class of methods known by name Accelerated Lambda Iteration. The existing computer codes, and some of the most useful grids of model atmospheres that are publicly available, are briefly summarized. Some interesting properties of newly computed NLTE models atmospheres and their comparison to LTE models are shown. Finally, it is briefly shown how the model atmospheres are used to determine basic stellar parameters.
|Original language||English (US)|
|Title of host publication||Planets, Stars and Stellar Systems Volume 4|
|Subtitle of host publication||Stellar Structure and Evolution|
|Number of pages||35|
|State||Published - Jan 1 2013|
ASJC Scopus subject areas
- Physics and Astronomy(all)