Revealing the pulsational properties of the V777 Herculis star KUV 05134+2605 by its long-term monitoring
<b>Context.</b> KUV 05134+2605 is one of the 21 pulsating DB white dwarfs (V777 Her or DBV variables) known so far. The detailed investigation of the short-period and low-amplitude pulsations of these relatively faint targets requires considerable observational efforts from the ground, l...
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| Autores principales: | Bognár, Z., Paparó, M., Córsico, Alejandro Hugo, Kepler, S.O., Gyorffy, A. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2014
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/85146 |
| Aporte de: |
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