The Lyman α line wing

Details The Lyman α line wing The Lyman α line wing

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990aipc..216..604a&link_type=abstract

Spectral line shapes. AIP Conference Proceedings, Volume 216, pp. 604-604 (1990).

Physics

Line Shapes, Widths, And Shifts, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

Resonance broadening in the far wind of Lyman α is analyzed with
an expansion in of atomic hydrogen density and the interatomic potential
of H2. The extreme far wing profiles for hydrogen-rich DA white dwarf
stars are estimated. (AIP)

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