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:
| Publicado: |
2016
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v830_n2_p_Fontenla http://hdl.handle.net/20.500.12110/paper_0004637X_v830_n2_p_Fontenla |
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