On the orbital period of the cataclysmic variable V767 CYG
We present a photometric and spectroscopic study that helps to constrain the orbital period of the system V767 Cyg for the first time. From the analysis of the V filter light curve besides of that for the radial velocity curve for different Balmer series lines, we find a most likely orbital period o...
| Autores: | , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2018 |
| País: | México |
| Institución: | Universidad Autónoma de Nuevo León |
| Repositorio: | Redalyc-UANL |
| OAI Identifier: | oai:redalyc.org:57171627010 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57171627010 https://www.redalyc.org/journal/571/57171627010/ https://www.redalyc.org/journal/571/57171627010/html/ https://www.redalyc.org/journal/571/57171627010/57171627010.epub https://www.redalyc.org/journal/571/57171627010/movil |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas Novae stars: general cataclysmic variables stars: individual: V767 Cyg |
| Sumario: | We present a photometric and spectroscopic study that helps to constrain the orbital period of the system V767 Cyg for the first time. From the analysis of the V filter light curve besides of that for the radial velocity curve for different Balmer series lines, we find a most likely orbital period of 0.165 ± 0.012 days for the binary system. The data we present were obtained during two different observational campaigns. |
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