Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae
Accreting white dwarfs (WDs) in cataclysmic variables (CVs) show short-period (tens of minutes) brightness variations that are consistent with nonradial oscillations similar to gravity ( g ) modes observed in isolated WDs. The dwarf nova GW Librae was the first CV in which nonradial oscillations wer...
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| Hlavní autoři: | , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
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IOP Publishing
2023-01-01
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| Edice: | The Astrophysical Journal |
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| On-line přístup: | https://doi.org/10.3847/1538-4357/acd1df |
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