The MUSCLES Treasury Survey. IV. Scaling Relations for Ultraviolet, Ca II K, and Energetic Particle Fluxes from M Dwarfs
Characterizing the UV spectral energy distribution (SED) of an exoplanet host star is critically important for assessing its planet's potential habitability, particularly for M dwarfs, as they are prime targets for current and near-term exoplanet characterization efforts and atmospheric models...
Guardado en:
| Autores principales: | Buccino, Andrea Paola, Mauas, Pablo J.D., Vieytes, Mariela C. |
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| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v843_n1_p_Youngblood http://hdl.handle.net/20.500.12110/paper_0004637X_v843_n1_p_Youngblood |
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