Quasi-molecular line satellites in the far wing of the atomic hydrogen Balmer alpha spectral line

Details Quasi-molecular line satellites in the far wing of the atomic hydrogen Balmer alpha spectral line Quasi-molecular line satellites in the far wing of the atomic hydrogen Balmer alpha spectral line

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..213l&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

New theoretical calculations of the total profile of the atomic hydrogen Balmer alpha spectral line perturbed by collisions with protons and neutral hydrogen have been made using accurate theoretical molecular potentials to describe the interaction between radiator and perturber. We point out the possible existence of quasi-molecular features due to H-H+ and H-H. Measurements of the main ones in the spectrum of a plasma confirm the theoretical predictions.

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