The luminosity function in the solar neighbourhood

van Rhijn’s method is used to derive the luminosity function in the solar neighbourhood from large proper motion stars. The values obtained are smaller than the currently accepted ones; for M_B < 9, the factor is of the order of two. It is shown that these differences arise from the systematic er...

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Guardado en:
Detalles Bibliográficos
Autor principal: Muzzio, Juan Carlos
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1973
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/98701
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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