Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIX. NA X spectral lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIX. NA X spectral lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. XIX. NA X spectral lines

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..130..539d&link_type=abstract

Astronomy and Astrophysics Supplement, v.130, p.539-540

Astronomy and Astrophysics

Astrophysics

5

Lines: Profile-Atomic Data

Scientific paper

Using a semiclassical perturbation approach, we have calculated electron-, proton-, and He III-impact line widths and shifts for 57 Na X multiplets for perturber densities 10(17) - 10(24) cm(-3) and temperatures T 200 000 - 5 000 000 K. For lower perturber densities, the Stark broadening parameters are proportional to the perturber density. Table 1 is only available in electronic form: The material published electronically can be accessed: by ftp at cdsarc.u-strasbg.fr or 130.79.128.5 or on WWW at: http//cdsweb.u-strasbg.fr/Abstract.html

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