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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Detalles Bibliográficos
Autores principales: Gómez, A., Jaschek, Carlos
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1970
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/97849
Aporte de:
id I19-R120-10915-97849
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Gómez, A.
Jaschek, Carlos
The velocity ellipsoid for giants and dwarfs
topic_facet Astronomía
Galaxias
description 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 published ones. The complete paper will be published elsewhere.
format Articulo
Comunicacion
author Gómez, A.
Jaschek, Carlos
author_facet Gómez, A.
Jaschek, Carlos
author_sort Gómez, A.
title The velocity ellipsoid for giants and dwarfs
title_short The velocity ellipsoid for giants and dwarfs
title_full The velocity ellipsoid for giants and dwarfs
title_fullStr The velocity ellipsoid for giants and dwarfs
title_full_unstemmed The velocity ellipsoid for giants and dwarfs
title_sort velocity ellipsoid for giants and dwarfs
publishDate 1970
url http://sedici.unlp.edu.ar/handle/10915/97849
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