Building reliable models of M dwarf chromospheres: The impact of the usual assumptions

We study different approximations usually made to simplify the calculation of chromospheric models of M dwarf stars. The approximations we discuss in details are: the assumption that the minority species are in LTE, the omission of the contribution of numerous atomic and molecular lines (line blanke...

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Detalles Bibliográficos
Publicado:	1998
Materias:	Stars: atmospheres Stars: chromosphere Stars: late-type
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v336_n1_p281_Falchi http://hdl.handle.net/20.500.12110/paper_00046361_v336_n1_p281_Falchi
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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