ON THE SIGNIFICANCE OF STARK LINE SHIFTS FOR ELEMENT ABUNDANCE DETERMINATIONS BY THE MODEL ATMOSPHERE METHOD

Authors
KHOKHLOVA VL
Citation
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
Citations number
8
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Astronomy letters → ACNP
ISSN journal
10637737
Volume
20
Issue
1
Year of publication
1994
Pages
89 - 90
Database
ISI
SICI code
1063-7737(1994)20:1<89:OTSOSL>2.0.ZU;2-B
Abstract
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.