First observations of CN (2-1), HCO+ (3-2) and C2H (3-2) emission lines in the Perseus cluster: constraints on heating mechanisms in the cluster gas Molecules as heating probe in Perseus (2011)
Attributed to:
Star Formation and Protoplanetary Discs
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.19304.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.19304.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1