Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..212g&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 1, p. 212-214.
Astronomy and Astrophysics
Astrophysics
11
Abundance, Interstellar Chemistry, Interstellar Matter, Molecular Clouds, Nitric Oxide, Astronomical Models, Chemical Composition, Density Distribution, Line Spectra
Scientific paper
We report the detection of nitric oxide, NO, in the dark cloud TMC 1; the column density is 2.7 +/- 0.5 x 10 exp 14/sq cm resulting in a fractional abundance relative to H2 of NO concentration of 2.7 x 10 exp -8, a factor eight less than in L134N, a dark cloud where NO has been previously observed. This large difference in abundance for a simple molecule is reproduced in two types of models of interstellar chemistry: (1) models at steady state with different depletions factors for C, N and O; (2) models with constant depletions but including mixing processes with largely different time scales. These two effects contribute probably to enhance the chemical differences between dark clouds, and throughout an individual cloud.
Casoli Fabienne
Gerin Maryvonne
Viala Yves
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