The mass function in spectroscopic binaries

The distribution of the mass function of bright spectroscopic binaries is studied for systems with dwarf and with giant primaries. It is found that the distribution is very similar in both cases. Assuming that the inclination has a random distribution and postulating different distribution functions...

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Detalles Bibliográficos
Autores principales: Jaschek, Carlos, Ferrer, Osvaldo Eduardo
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1973
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/98698
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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