Stark Broadening of the Spectral Lines of Ne V

Details Stark Broadening of the Spectral Lines of Ne V Stark Broadening of the Spectral Lines of Ne V

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apjs..170..243h&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 170, Issue 1, pp. 243-250.

Astronomy and Astrophysics

Astronomy

7

Atomic Data, Atomic Processes, Line: Profiles

Scientific paper

Using a semiclassical approach, we have calculated ab initio electron-, proton-, and ionized helium-impact line widths and shift for 26 Ne V multiplets. Energy levels and oscillator strengths have been calculated using SUPERSTRUCTURE code. Results have been presented for an electron density of 1017 cm-3 as a function of temperature, and are compared with experimental and other theoretical results.

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