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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)

First Author: Traficante A

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