Article contents
Pulsating white dwarfs in cataclysmic variables: The marriage of ZZ Cet and dwarf nova
Published online by Cambridge University Press: 12 April 2016
Abstract
There are now four dwarf novae known with white dwarf primaries that show large amplitude non-radial oscillations of the kind seen in ZZ Cet stars. We compare the properties of these stars and point out that by the end of the Sloan Digital Sky Survey more than 30 should be known.
- Type
- Part 6. Binary stars and pulsation
- Information
- International Astronomical Union Colloquium , Volume 193: Variable Stars in the Local Group , 2004 , pp. 382 - 386
- Copyright
- Copyright © Astronomical Society of the Pacific 2004
References
- 5
- Cited by