Biblio
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Filtres: Mot-clé is Galaxy: structure and Auteur is Compiègne, M. [Clear All Filters]
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\deg, 0\deg),
, \mnras, jun, Volume 440, p.3588-3612, (2014)
