Stark broadening effect and zirconium conflict problem

Details Stark broadening effect and zirconium conflict problem Stark broadening effect and zirconium conflict problem

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..559..208d&link_type=abstract

SPECTRAL LINE SHAPES: Volume 11, 15th ICSLS. AIP Conference Proceedings, Volume 559, pp. 208-210 (2001).

Astronomy and Astrophysics

Astrophysics

Stellar Characteristics And Properties

Scientific paper

Using the Modified Semiempirical Method we have calculated the electron-impact widths for four singly and doubly ionized zirconium UV lines of astrophysical importance. Using the SYNTH and ATLAS9 codes for stellar atmospheres similar to that of the HgMn star χ Lupi we have synthesized the line profiles and found equivalent widths for these lines. The influence of the Stark broadening effect on abundance determination and its contribution to the so-called ``zirconium conflict'' are discussed. .

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