Chlorine-Bearing Molecules in Cold and Warm Interstellar Clouds

Details Chlorine-Bearing Molecules in Cold and Warm Interstellar Clouds Chlorine-Bearing Molecules in Cold and Warm Interstellar Clouds

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996em%26p...73..133a&link_type=abstract

Earth, Moon and Planets, Volume 73, Issue 2, pp.133-145

Physics

2

Scientific paper

A new time-dependent model of chlorine chemistry in cold and warm TMC-1 and Orion clouds was constructed using results of recent laboratory and theoretical studies on the reaction of chlorine molecules. The chemistry of chlorine was found to be fairly simple in dense interstellar clouds. Only the species Cl and HCl have a significant fractional abundance. Our results for the HCl molecule are in agreement with those obtained from the observation and from theoretical values of Orion cloud.

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