The pros and cons of the inversion method approach to derive 3D dust emission properties in the ISM: the Hi-GAL field centred on (l, b) = (30 , 0 ) (2014)
Attributed to:
The Radio Universe: astronomy and astrophysics at the Jodrell Bank Centre for Astrophysics 2014-2017
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stu493
Publication URI: http://dx.doi.org/10.1093/mnras/stu493
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4