Influence of ion-atom collisions on the absorption of radiation in white dwarfs

Details Influence of ion-atom collisions on the absorption of radiation in white dwarfs Influence of ion-atom collisions on the absorption of radiation in white dwarfs

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...256..305m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 256, no. 1, p. 305-308.

Astronomy and Astrophysics

Astrophysics

14

Atomic Collisions, Helium Ions, Ionic Collisions, Radiation Absorption, Stellar Spectra, White Dwarf Stars, Absorption Spectra, Continuous Spectra, Stellar Radiation

Scientific paper

In order to provide the relevant absorption coefficients for the interpretation of the continuum absorption spectra in a number of white dwarfs with helium dominated atmospheres, the processes He2(+) (omega) yields He + He(+) and He + He(+) + h(omega) yields He + He(+) have been considered together. We present also the absorption coefficients for the conditions of DA white dwarf atmospheres calculated by taking into account together the processes H2(+) + h(omega) yields H + H(+) and H+H(+) + h(omega) yields H + H(+).

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