Long-term decrease and cyclic variation in the orbital period of the eclipsing dwarf nova V2051 OPH
V2051 Oph is a deeply eclipsing dwarf nova with an orbital period below the period gap of cataclysmic variables (CVs). It has been photometrically monitored since 2008 June and 24 mid-eclipse times of the white dwarf have been obtained. The changes in the orbital period are investigated using all of...
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| Autores principales: | Qian, S. B., Han, Z. T., Fernández Lajús, Eduardo, Zhu, L. Y., Li, L. J., Liao, W. P., Zhao, E. G. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2015
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86916 |
| Aporte de: |
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