Issue |
A&A
Volume 381, Number 1, JanuaryI 2002
|
|
---|---|---|
Page(s) | L13 - L16 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20011544 | |
Published online | 15 January 2002 |
Letter to the Editor
A network for interstellar CO – The first application of objective reduction techniques in astrochemistry
1
School of Chemistry, University of Leeds, Leeds LS2 9JT, UK
2
Department of Physics and Astronomy, University of Leeds, Leeds LS2 9JT, UK
3
Departments of Physics and Astronomy, Ohio State University, Columbus OH, 43210-1106, USA
T. W. Hartquist
Received:
24
September
2001
Accepted:
6
November
2001
A reduced network for CO production and removal, obtained via the use of objective techniques, is shown to produce reliable results over a wide range of physical conditions. Our analysis indicates that reactions involving species with long carbon chains are important in governing the CO abundance in some translucent regions.
Key words: molecular processes / stars: formation / ISM: abundances / ISM: clouds / ISM: molecules
© ESO, 2002
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