Stark broadening of spectral lines of multicharged ions of astrophysical interest. I - C IV lines. II - SI IV lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. I - C IV lines. II - SI IV lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. I - C IV lines. II - SI IV lines

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...89..581d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 89, no. 3, Sept. 1991, p. 581-598. Research supported by Obs

Astronomy and Astrophysics

Astrophysics

100

Carbon, Line Spectra, Perturbation Theory, Quantum Mechanics, Stark Effect, Atomic Energy Levels, Electron Impact, Ionized Gases, Space Plasmas

Scientific paper

Results are presented on calculations of the electron-, proton-, and ionized helium-impact line widths and shifts for 31 C IV multiplets and 40 Si IV multiplets. These data are compared with observations and are used to investigate the Stark broadening parameter regularities within the spectral series. For both the C IV and Si IV multiplets, a gradual change of the Stark widths was obtained. The reason for this is discussed.

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