Frecuencia de binarias espectroscópicas en tipos espectrales B, A y K
The procedure of Petrie (1960) for deriving the proportion of spectroscopic binaries was improved and applied to the samples of stars of table I, where also the final results are given. Some selection effects were considered. The discussion in full will be published elsewhere.
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1969
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/95374 |
| Aporte de: |
| Sumario: | The procedure of Petrie (1960) for deriving the proportion of spectroscopic binaries was improved and applied to the samples of stars of table I, where also the final results are given. Some selection effects were considered. The discussion in full will be published elsewhere. |
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