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Observation of a Variable, ZZ Ceti White Dwarf: GD154
Published online by Cambridge University Press: 12 April 2016
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The ZZ Ceti stars form a class of variable white dwarfs: the hydrogen dominated atmosphere ones, which do pulsate in an instability strip in the effective temperature range 13000K-11500K. We know 22 such ZZ Ceti white dwarfs. Their variations are caused by nonradial g-mode pulsations with periods are in the range 100-1000 seconds.
A subsample of the ZZ Ceti stars shows amplitude variations on time scales of the order of one month. These variations could be driven by nonlinear phenomena.
- Type
- II. Observational Facts
- Information
- International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 201 - 204
- Copyright
- Copyright © Kluwer 1993
References
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