Stark broadening of spectral lines of multicharged ions of astrophysical interest. IV - N V lines. V - SC III and TI IV lines

Details Stark broadening of spectral lines of multicharged ions of astrophysical interest. IV - N V lines. V - SC III and TI IV lines Stark broadening of spectral lines of multicharged ions of astrophysical interest. IV - N V lines. V - SC III and TI IV lines

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...95..109d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 95, no. 1, p. 109-128.

Astronomy and Astrophysics

Astrophysics

25

Astronomical Spectroscopy, Interstellar Gas, Molecular Ions, Spectral Line Width, Stark Effect, Coulomb Collisions, Helium, Stellar Atmospheres, Line Profile, Atomic Data, Stark Broadening

Scientific paper

Using a semiclassical approach, we have calculated electron-, proton-,
and ionized helium-impact line widths and shifts for 30 N V multiplets.
The obtained data have been compared with the existing experimental
values.

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