New Computation Of The Astrophysical HD-Cooling Function

Details New Computation Of The Astrophysical HD-Cooling Function New Computation Of The Astrophysical HD-Cooling Function

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944305s&link_type=abstract

American Astronomical Society, AAS Meeting #219, #443.05

Astronomy and Astrophysics

Astrophysics

Scientific paper

New thermal rate coefficients for rotational transitions in HD+o-/p-H2 collisions will be presented. Extensive quantum mechanical coupled-channel calculation has been performed. Recently published H2-H2 potential energy surfaces have been applied. Astrophysical HD-cooling function at low-density-limit due to HD+o-/p-H2 collisions is computed with the use of the new thermal rate coefficients. A comparison and analysis with previous results will also be presented.

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