Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXIII. Be III

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXIII. Be III Stark broadening of spectral lines of multicharged ions of astrophysical interest. XXIII. Be III

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...400..791d&link_type=abstract

Astronomy and Astrophysics, v.400, p.791-793 (2003)

Astronomy and Astrophysics

Astrophysics

3

Lines: Profiles, Atomic Data, Atomic Processes, Line: Formation

Scientific paper

Using a semiclassical perturbation method, we have calculated electron-, proton-, and ionized helium-impact line widths and shifts for 52 Be III multiplets as a function of temperature and perturber density. Electron temperatures are 10 000 K; 20 000 K; 50 000 K; 100 000 K; 200 000 K and 300 000 K and perturber densities are from 1011 cm-3 up to 1021 cm-3. The obtained results have been used for discussion of regularities and systematic trends along spectral series.
Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?/A+A/400/791

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