Stark broadening of He II lines

Details Stark broadening of He II lines Stark broadening of He II lines

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...78...51s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 78, no. 1, April 1989, p. 51-87.

Astronomy and Astrophysics

Astrophysics

79

Astronomical Spectroscopy, Helium, Line Spectra, Stark Effect, Tables (Data), Balmer Series, Electron Trajectories, Ion Charge, Paschen Series, Spectral Line Width, Unified Field Theory

Scientific paper

Results for the Stark broadening of He-II lines of the Balmer, Paschen, and Pickering series under conditions of astrophysical interest are given in tabular form. The data have been calculated using the unified theory of Vidal et al. (1970), and they take into account the effects of the ionic charge on the paths of the electrons. Stark functions have been tabulated for densities ranging on a logarithmic scale from 3.162 x 10 to the 10th/cu cm to 1 x 10 to the 16th/cu cm and for temperatures from 10,000-320,000 K.

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