The near-ultraviolet luminosity function of young, early M-type dwarf stars

Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magnetohydrodynamic dynamos during stellar youth. Near-ultraviolet (NUV) irradiation can erode and alter the chemistry of planetary atmospheres, and a quantitative...

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Detalles Bibliográficos
Autores principales:	Ansdell, M., Gaidos, E., Mann, A.W., Lépine, S., James, D., Buccino, A., Baranec, C., Law, N.M., Riddle, R., Mauas, P., Petrucci, R.
Formato:	JOUR
Materias:	Binaries: Close Stars: Activity Stars: Late-type Stars: Luminosity function, mass function
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v798_n1_p_Ansdell
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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