The CH radical in diffuse interstellar clouds

Observations of the interstellar CH A-X R2(1) line at 4300.3 A are presented for 29 lines of sight extending from 140 to 2800 pc in the Galactic plane. A comparison of the CH and H2 column density shows that N(CH) varies as N(H2) as expected for production of CH by a gas phase reaction network runni...

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Published in:Astronomy and astrophysics (Berlin) 1984, Vol.130 (1), p.62-66
Main Authors: DANKS, A. C, FEDERMAN, S. R, LAMBERT, D. L
Format: Article
Language:English
Subjects:
Astronomy
Earth, ocean, space
Exact sciences and technology
Interstellar medium (ism) and nebulae in milky way
Molecular clouds, h2 clouds, dense clouds, and dark clouds
Stellar systems. Galactic and extragalactic objects and systems. The universe
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container_title Astronomy and astrophysics (Berlin)
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creator DANKS, A. C
FEDERMAN, S. R
LAMBERT, D. L
description Observations of the interstellar CH A-X R2(1) line at 4300.3 A are presented for 29 lines of sight extending from 140 to 2800 pc in the Galactic plane. A comparison of the CH and H2 column density shows that N(CH) varies as N(H2) as expected for production of CH by a gas phase reaction network running in molecular hydrogen. The network also reproduces the observed ratio N(CH)/N(H2) for these diffuse interstellar clouds.
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subjects Astronomy
Earth, ocean, space
Exact sciences and technology
Interstellar medium (ism) and nebulae in milky way
Molecular clouds, h2 clouds, dense clouds, and dark clouds
Stellar systems. Galactic and extragalactic objects and systems. The universe
title The CH radical in diffuse interstellar clouds
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