Determination of the Mass Loss Rate and the Terminal Velocity of Stellar Winds. I. Genetic Algorithm for Automatic Line Profile Fitting
A new method for automatic fitting of P Cyg line profiles in UV spectra ofstellar winds is presented. The line source function is calculated using Sobolev`sapproximation and the emergent flux is obtained by exact integration of the equation of the radiation transport (similar to the SEI method descr...
Na minha lista:
| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Principais autores: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2005
|
| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57141114 |
| Tags: |
Sem tags, seja o primeiro a adicionar uma tag!
|