Molecules in white dwarfs

Details Molecules in white dwarfs Molecules in white dwarfs

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.147..107g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 147, no. 1, Aug. 1988, p. 107-113.

Astronomy and Astrophysics

Astrophysics

8

Gas Dissociation, Molecular Gases, Stellar Atmospheres, White Dwarf Stars, Abundance, Atmospheric Models, Helium, Hydrogen, Positive Ions

Scientific paper

Molecular dissociation equilibria have been determined for model atmospheres of DA and non-DA white dwarfs. Elemental abundances have been obtained for effective temperatures ranging from 5500-20,000 K. It is found that He2(+) and HeH(+) are the most abundant molecules in the atmospheres of non-DA white dwarfs and that H2 and H2(+) are the most abundant molecules in DA white dwarfs.

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