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09 February 2025
 
  » arxiv » astro-ph/0702067

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Velocity Fields at the Surface of ZZ Ceti Stars
D. Koester ; E. Kompa ;
Date 2 Feb 2007
AbstractWe demonstrate that the peculiar line profiles observed in DA white dwarfs in the temperature range of the ZZ Ceti variables can be explained by the surface velocity fields associated with the pulsations.
Source arXiv, astro-ph/0702067
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