Stimulated Radiative Association of He and H^+

Details Stimulated Radiative Association of He and H^+ Stimulated Radiative Association of He and H^+

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...508..151z&link_type=abstract

The Astrophysical Journal, Volume 508, Issue 1, pp. 151-156.

Astronomy and Astrophysics

Astronomy

18

Atomic Processes, Cosmology: Early Universe, Molecular Processes, Ism: Planetary Nebulae: General, Galaxies: Quasars: General

Scientific paper

The enhancement of the rate coefficient for the radiative association of He and H^+ to form HeH^+ arising from stimulated emission due to a blackbody radiation field is calculated. The effects on the fractional abundance of HeH^+ in the early universe, in supernova ejecta, and in planetary nebulae are small. There may occur some enhancement in the abundance of HeH^+ in quasar broad-line clouds.

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