H-alpha line profiles in DA white dwarfs

Astronomy and Astrophysics – Astronomy

Scientific paper

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H Alpha Line, Line Spectra, Stellar Atmospheres, Stellar Rotation, White Dwarf Stars, Cool Stars

Scientific paper

Rotational velocities have been determined for several white dwarfs from the sharp NLTE core of the Hα profile. A new synthetic profile has been computed for Teff = 16,000K, log g = 8.0 white dwarfs; this profile fits closely the observed spectra of white dwarfs of this temperature. The authors confirm that Wolf 485A rotates with a velocity v sin i = 42±9 km s-1. Rotational velocities in 40 Eri B, SA 29-130, and L970-30 are less than 20 km s-1.

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