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The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 µm surface brightness ratios (2015)

First Author: Bendo G

Attributed to: Support for the UK ALMA Regional Centre Node funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stu1841

Publication URI: http://dx.doi.org/10.1093/mnras/stu1841

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1