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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)

First Author: Bayet E

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