Vl. Khokhlova, ON THE SIGNIFICANCE OF STARK LINE SHIFTS FOR ELEMENT ABUNDANCE DETERMINATIONS BY THE MODEL ATMOSPHERE METHOD, Astronomy letters, 20(1), 1994, pp. 89-90
While determining chemical abundances in the atmospheres of magnetic,
chemically peculiar stars by the model atmosphere method, one should t
ake into account die shifts of spectral lines caused by collisions wit
h electrons.