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...
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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autoři: | , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2005
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57141114 |
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