The explanation of the 1400 and 1600 A features in DA white dwarfs

Details The explanation of the 1400 and 1600 A features in DA white dwarfs The explanation of the 1400 and 1600 A features in DA white dwarfs

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142l...5k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 1, Jan. 1985, p. L5-L8.

Astronomy and Astrophysics

Astronomy

58

Absorption Spectra, Iue, Stellar Spectra, Ultraviolet Astronomy, White Dwarf Stars, Hydrogen Ions, Molecular Absorption, Molecular Ions

Scientific paper

The authors present new IUE observations of 4 cool DA white dwarfs together with additional data for 8 objects from the literature. All objects show absorption features near 1400 and/or 1600 Å, which were already noted by other authors. These features are explained as due to quasi-molecular absorption of the H2 (1600 Å) resp. H2+ (1400 Å) molecules.

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