The velocity ellipsoid for giants and dwarfs

The solar motion and the velocity ellipsoid are derived from samples of stars of different spectral types and luminosity class. The equations used are those of the radial velocity component of motion, including the K-term and galactic rotation corrections. The results obtained are compared with the...

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Guardado en:
Detalles Bibliográficos
Autores principales: Gómez, A., Jaschek, Carlos
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1970
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/97849
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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