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...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1970
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/97849 |
| Aporte de: |
| Sumario: | 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. |
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