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H3+ in diffuse interstellar gas
Authors:Cesare Cecchi-Pestellini  Alexander Dalgarno
Institution:Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA; Dipartimento di Astronomia e Scienza dello Spazio, Universitádi Firenze, Largo E. Fermi 5, 50125 Firenze, Italy
Abstract:A model is constructed of the material in front of the star Cygnus OB2 no. 12 in which dense cores are embedded in diffuse clumps of gas. The model reproduces the measured abundances of C2 and CO, and predicts a column density of 91010 cm2 for HCO+.
Keywords:molecular processes  ISM: clouds  ISM: molecules
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