Pulsations driven by the ε-mechanism in post-merger remnants: First results
Helium-rich subdwarfs are a rare subclass of hot subdwarf stars which constitute a small and inhomogeneous group showing varying degrees of helium enrichment. Only one star, LS IV º14 116 has been found to show multiperiodic luminosity variations. The variability of LS IV º14 116 has been explained...
Guardado en:
| Autores principales: | Miller Bertolami, Marcelo Miguel, Córsico, Alejandro Hugo, Zhang, X., Althaus, Leandro Gabriel, Jeffery, C.S. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2013
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/85574 |
| Aporte de: |
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