Starting model for photospheres of late-type stars
A starting temperature distribution for the computation of model atmospheres including convection is proposed. To solve the transfer problem we used an iterative method based on a Feautrier-type computing scheme. We find that the starting model yields satisfactory convergence to the solution of the...
Guardado en:
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1994
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/155114 |
| Aporte de: |
| Sumario: | A starting temperature distribution for the computation of model atmospheres including convection is proposed. To solve the transfer problem we used an iterative method based on a Feautrier-type computing scheme. We find that the starting model yields satisfactory convergence to the solution of the transfer equation. |
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