SEMI-EMPIRICAL MODELING of the PHOTOSPHERE, CHROMOPSHERE, TRANSITION REGION, and CORONA of the M-DWARF HOST STAR GJ 832
Stellar radiation from X-rays to the visible provides the energy that controls the photochemistry and mass loss from exoplanet atmospheres. The important extreme ultraviolet (EUV) region (10-91.2 nm) is inaccessible and should be computed from a reliable stellar model. It is essential to understand...
Guardado en:
| Autores principales: | Fontenla, J.M., Linsky, J.L., Witbrod, J., France, K., Buccino, A., Mauas, P., Vieytes, M., Walkowicz, L.M. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v830_n2_p_Fontenla |
| Aporte de: |
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