Broadening due to collisions with charged particles of V V and V XIII spectral lines.

Details Broadening due to collisions with charged particles of V V and V XIII spectral lines. Broadening due to collisions with charged particles of V V and V XIII spectral lines.

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pobeo..57...15d&link_type=abstract

Publications of the Astronical Observatory of Belgrade, No. 57, p. 15 - 18

Astronomy and Astrophysics

Astronomy

Spectral Lines: Stark Broadening, Spectral Lines: Vanadium

Scientific paper

Using a semi-classical approach, the authors have calculated electron-, proton-, and He III-impact line widths and shifts for 33 vanadium V multiplets, for perturber densities 1014 - 1021cm-3 and temperatures T = 50,000 - 500,000K, and 26 vanadium XIII multiplets, for perturber densities 1018 - 1022cm-3 and temperatures T = 500,000 - 5,000,000K.

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