ε-mechanism driven pulsations in hot subdwarf stars with mixed H-He atmospheres
The ε mechanism is a self-excitation mechanism of stellar pulsations which acts in regions where nuclear burning takes place. It has been shown that the ε mechanism can excite pulsations in hot pre-horizontal branch stars before they settle into the stable helium core-burning phase and that the shor...
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| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
De Gruyter
2017-12-01
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| coleção: | Open Astronomy |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.1515/astro-2017-0431 |
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