Stark Broadening of BIII Lines of Astrophysical Interest

Details Stark Broadening of BIII Lines of Astrophysical Interest Stark Broadening of BIII Lines of Astrophysical Interest

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..101..583d&link_type=abstract

Astronomy and Astrophysics Supplement, Vol.101, NO. 3/NOVI, P. 583, 1993

Astronomy and Astrophysics

Astrophysics

7

Lines, Profile, Atomic And Molecular Data, Hg-Mn Stars

Scientific paper

We report here results of Bi II spectral line Stark broadening research within a modified semi-empirical approach. The strong absorption Bi II lines observed in Hg-Mn star atmospheres have been investigated, as well as other Bi II lines of importance for astrophysical and laboratory plasma. Stark width and shift data for 26 Bi II lines are presented as a function of temperature. The obtained results have been compared with experiments and with other estimations.

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