Multiple perturber effects in the far red wing of Lyman α line

Details Multiple perturber effects in the far red wing of Lyman α line Multiple perturber effects in the far red wing of Lyman α line

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1058..326a&link_type=abstract

SPECTRAL LINE SHAPES: Volume 15-19th International Conference on Spectral Line Shapes. AIP Conference Proceedings, Volume 1058,

Physics

Line Shapes, Widths, And Shifts, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Low Luminosity Stars, Subdwarfs, And Brown Dwarfs

Scientific paper

A small fraction of the DA white dwarf are known to have rather low effective temperature. It is of considerable interest to determine line profiles in these extreme physical conditions. In such cool white dwarfs the perturber density is so high that the one perturber approximation breaks down and the collisional effects must be treated by using the autocorrelation formalism in order to take account the simultaneous collisions with more than one perturbing atom.

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