Stark broadening of Ca II spectral lines

Details Stark broadening of Ca II spectral lines Stark broadening of Ca II spectral lines

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jqsrt..49..157d&link_type=abstract

Journal of Quantitative Spectroscopy & Radiative Transfer (ISSN 0022-4073), vol. 49, no. 2, p. 157-164.

Computer Science

9

Calcium, Line Spectra, Spectral Line Width, Stellar Spectra, Resonance Lines, Stellar Spectrophotometry

Scientific paper

The semiclassical-perturbation formalism is used to calculate electron-,
proton, and ionized-helium-impact line widths and shifts for 28 Ca II
multiplets. Data obtained are compared with experimental and theoretical
results.

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