Atmospheric models of flare stars: The flaring state of AD Leonis
We compute a set of semi-empirical atmospheric models for a large flare on the dMe star AD Leo, assuming different filling factors. These are the first models computed to match both the continuum observations, and a wide set of chromospheric spectral lines. We found that the models with a filling fa...
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| Autores principales: | Mauas, P.J.D., Falchi, A. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v310_n1_p245_Mauas |
| Aporte de: |
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