Spectroscopic study of RU Eridani
The eclipsing binary RU Eri (P=0.63 d; V=9.35 m) was observed spectroscopically from CTIO with a dispersion of 43 Å/mm in the blue and 86 Å/mm in Hα. We analyzed the radial velocity plots and we derived the orbital elements for the primary component. A model for the system is proposed.
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1987
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/141511 |
| Aporte de: |
| Sumario: | The eclipsing binary RU Eri (P=0.63 d; V=9.35 m) was observed spectroscopically from CTIO with a dispersion of 43 Å/mm in the blue and 86 Å/mm in Hα. We analyzed the radial velocity plots and we derived the orbital elements for the primary component. A model for the system is proposed. |
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