C2absorption-line diagnostics of diffuse interstellar clouds

DSpace/Manakin Repository

C2absorption-line diagnostics of diffuse interstellar clouds

Citable link to this page


Title: C2absorption-line diagnostics of diffuse interstellar clouds
Author: Cecchi-Pestellini, Cesare; Dalgarno, Alexander

Note: Order does not necessarily reflect citation order of authors.

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.
Full Text & Related Files:
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.
Published Version: doi:10.1046/j.1365-8711.2002.05418.x
Terms of Use: This article is made available under the terms and conditions applicable to Other Posted Material, as set forth at http://nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of-use#LAA
Citable link to this page: http://nrs.harvard.edu/urn-3:HUL.InstRepos:30403734
Downloads of this work:

Show full Dublin Core record

This item appears in the following Collection(s)


Search DASH

Advanced Search