New study of the quasi-molecular Lyman ϒ satellites due to H-H collisions

Details New study of the quasi-molecular Lyman ϒ satellites due to H-H collisions New study of the quasi-molecular Lyman ϒ satellites due to H-H collisions

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007uasb.conf..173a&link_type=abstract

UV Astronomy: Stars from Birth to Death. Proceedings of the Joint Discussion n.4 during the IAU general Assembly of 2006. Ana I.

Astronomy and Astrophysics

Astronomy

Uv Astronomy, Line Profiles, Stars: White Dwarfs

Scientific paper

Structures observed about 995 °A in the Lyman ϒ wing of hot
white dwarfs have been demonstrated to be due to quasi-molecular
absorption of H 2 molecules. We present new theoretical calculations of
the line profile of Lyman that include the variation of the radiative
dipole moment during the collision.

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