Article contents
Accretion Geometry of Synchronously Rotating Magnetic Cataclysmic Variables: Theories versus Observations
Published online by Cambridge University Press: 25 April 2016
Abstract
We review the magnetic locking of the white dwarf and the companion star in AM Herculis-type binaries for various white dwarf magnetic field structures, and compare the theoretical results with observations. The model in which the white dwarf has a dipole plus a quadrupole field is found to be in closest agreement with the recent observations.
- Type
- Galactic and Stellar
- Information
- Publications of the Astronomical Society of Australia , Volume 11 , Issue 2 , August 1994 , pp. 198 - 200
- Copyright
- Copyright © Astronomical Society of Australia 1994
References
- 2
- Cited by