Chemical Modelling of Molecular Sources - Part Two - L183

Details Chemical Modelling of Molecular Sources - Part Two - L183 Chemical Modelling of Molecular Sources - Part Two - L183

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..425m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 207, NO.2, P.425, 1984

Astronomy and Astrophysics

Astronomy

36

Scientific paper

We apply the chemical model described by us in Paper I to the dark dust cloud L183 (L134 N). This cloud shows similarities in density, temperature and extinction to TMC-1, but has much less abundances of several molecular species, including the cyanopolyynes, than TMC-1. We show that reasonable changes to the free parameters in our scheme, in particular the elemental depletions, can lead to calculated abundances which are in good agreement with the observations. The key details of the reaction scheme are discussed and some observational tests of the model are suggested.

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