Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae

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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Bibliographic Details
Main Authors: Praphull Kumar, Dean M. Townsley
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
White dwarf stars
Cataclysmic variable stars
Asteroseismology
Stellar oscillations
Classical novae
Online Access:https://doi.org/10.3847/1538-4357/acd1df

Internet

https://doi.org/10.3847/1538-4357/acd1df

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