Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXI. SC X, SC XI, TI XI and TI XII spectral lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXI. SC X, SC XI, TI XI and TI XII spectral lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXI. SC X, SC XI, TI XI and TI XII spectral lines

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..131..143d&link_type=abstract

Astronomy and Astrophysics Supplement, v.131, p.143-144

Astronomy and Astrophysics

Astrophysics

5

Lines: Profile, Atomic Data, Plasmas

Scientific paper

By using the semiclassical-perturbation formalism, we have calculated electron-, proton-, and He III-impact line widths and shifts for 4 Sc X, 10 Sc XI, 4 Ti XI and 27 Ti XII multiplets, significant for analysis, investigation and modeling of different plasmas in solar and stellar physics, physics and technology. The results are presented as a function of temperature and perturber density. Tables 1-4 are only available in electronic form at the CDS via anonymous ftp (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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