No CrossRef data available.
Article contents
Pulsations in white dwarf stars
Published online by Cambridge University Press: 18 February 2014
Abstract
We first present a brief description of the six distinct families of pulsating white dwarfs that are now known. These are all opacity-driven pulsators showing low- to mid-order, low-degree gravity modes. We then discuss some recent highlights that have come up in the field of white dwarf asteroseismology.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 273 - 280
- Copyright
- Copyright © International Astronomical Union 2014