Stark broadening of O V 1371 A˚ line in stellar atmospheres

Details Stark broadening of O V 1371 A˚ line in stellar atmospheres Stark broadening of O V 1371 A˚ line in stellar atmospheres

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1043..410d&link_type=abstract

EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP Conference Proceedings, Volume 1043, pp. 410-411 (2008).

Astronomy and Astrophysics

Astronomy

Normal Galaxies, Extragalactic Objects And Systems, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, Astronomical Observations, Magnetohydrodynamics And Plasmas, Photometric, Polarimetric, And Spectroscopic Instrumentation

Scientific paper

The Stark broadening parameters of O V 1371 A˚ spectral line, observed in stellar atmospheres of hot stars, determined within the semiclassical perturbation method, are used for the analysis of the importance of this broadening mechanism in white dwarf atmospheres. We found that Stark broadening mechanism is very important in such plasma conditions and should be taken into account.

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