Pulsational instability of high-luminosity H-rich pre-white dwarf star
We present a pulsational stability analysis on high-luminosity H-rich (DA) white dwarf models evolved from low-metallicity progenitors. We found that the ε mechanism due to H-shell burning is able to excite low-order g modes.
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| Hlavní autoři: | , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
EDP Sciences
2017-01-01
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| Edice: | EPJ Web of Conferences |
| On-line přístup: | https://doi.org/10.1051/epjconf/201715206012 |
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