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The decay of MG II emission in Main Sequence (MS) stars

Abstract:

Age decay of the 2800 A Mg II doublet in main sequence stars was studied, using IUE and literature data. The nonlinearity of the decay is confirmed. The emission shows a strong decrease until 2 times 10 to the 19th power years. Behavior of older stars is unclear.

Año de publicación:

1982

Keywords:

    Fuente:

    googlegoogle

    Tipo de documento:

    Other

    Estado:

    Acceso abierto

    Áreas de conocimiento:

    • Espectroscopia astronómica

    Áreas temáticas:

    • Cuerpos y fenómenos celestes específicos

    Contribuidores:

    Galo Cornejo GómezGalo Cornejo Gómez