The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 µm surface brightness ratios (2015)
Attributed to:
Astronomy Observation and Theory Consolidated Grant 2012
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