The influence of electron scattering on the He II line profiles in HD 50896

Details The influence of electron scattering on the He II line profiles in HD 50896 The influence of electron scattering on the He II line profiles in HD 50896

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...280..744h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 280, May 15, 1984, p. 744-748.

Other

55

Electron Scattering, Helium, Line Spectra, Stellar Spectra, Early Stars, Opacity, Stellar Atmospheres, Wolf-Rayet Stars

Scientific paper

An investigation into the effects of electron scattering on the He II line profiles in the spectrum of HD 50896 has been carried out. It is found that the red wing seen on the He II (7-4) line is due to electron scattering and not, as previously thought, an unidentified transition. The presence of a red electron scattering wing on other He II lines is confirmed by both observations and theoretical modeling.

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