Velocity Fields at the Surface of ZZ Ceti Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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4 pages, 4 figures, to be published in the proceedings of the 15th European Workshop on White Dwarfs (ASP)

Scientific paper

We 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.

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