Line broadening of HD immersed in He and H2 gas

Details Line broadening of HD immersed in He and H2 gas Line broadening of HD immersed in He and H2 gas

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...265..859s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 265, no. 2, p. 859-868.

Astronomy and Astrophysics

Astrophysics

3

Deuterium, Gas Giant Planets, Helium, Hydrogen, Planetary Atmospheres, Spectral Line Width, Abundance, Doppler Effect, Infrared Radiation, Molecular Collisions, S Matrix Theory

Scientific paper

Collision integrals have been calculated which determine the R(0) and R(1) line shapes of HD in He and H2 gas at temperatures up to 500 K (He) and 300 K (H2). The required scattering matrices have been obtained in close coupled calculations using an improved interaction potential of H2-H2 (F84) in the isotopic substituted form. The results are of interest in connection with the planned observations of atmospheres of the outer planets.

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