New Methods in Modeling of Hot Stellar Atmospheres
In the present study we had three main aims. First to study the possibility of reducing the initial model atmosphere data to short analytical polynomials. The second was to use as the depth variable the logarithm of the local gas pressure instead the Rosseland mean. The third aim was to check the ap...
Guardat en:
| Autors principals: | , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
De Gruyter
2013-06-01
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| Col·lecció: | Open Astronomy |
| Matèries: | |
| Accés en línia: | https://doi.org/10.1515/astro-2017-0155 |
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