Lyman gamma satellites due to H-H+ collisions: Application to FUSE observations of hot white dwarfs

Details Lyman gamma satellites due to H-H+ collisions: Application to FUSE observations of hot white dwarfs Lyman gamma satellites due to H-H+ collisions: Application to FUSE observations of hot white dwarfs

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..509b&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Lyman gamma profiles perturbed by protons using molecular potential of Peek allow us to identificate a large feature near 995 A in FUSE observations of hot white dwarfs. It is visible also in the HUT spectrum of Wolf1346 and in some ORFEUS spectra. This feature is due to Quasi-molecular Lyman gamma satellites due to H-H+ collisions near 991 and 996A.

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