Publication: C2absorption-line diagnostics of diffuse interstellar clouds
Loading...
Open/View Files
Date
2002
Published Version
Journal Title
Journal ISSN
Volume Title
Publisher
Oxford University Press (OUP)
The Harvard community has made this article openly available. Please share how this access benefits you.
Citation
Cecchi-Pestellini, Cesare, and Alexander Dalgarno. 2002. “C2absorption-Line Diagnostics of Diffuse Interstellar Clouds.” Monthly Notices of the Royal Astronomical Society 331 (3) (April): L31–L34. doi:10.1046/j.1365-8711.2002.05418.x.
Abstract
The excitation of the diatomic carbon molecule in diffuse interstellar clouds is discussed for a cloud with large density fluctuations of small linear filling factor along the line of sight. Possible implications for the chemistry of the diffuse cloud in front of Cygnus OB2 No. 12 are discussed.
Description
Other Available Sources
Research Data
Keywords
molecular processes, ISM: clouds, ISM: individual: Cygnus OB2 No. 12, ISM: molecules
Terms of Use
This article is made available under the terms and conditions applicable to Other Posted Material (LAA), as set forth at Terms of Service