Biblio
2 resultats trouvés
Filtres: Auteur is Fuller, G. A. [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)
Characterizing precursors to stellar clusters with Herschel,
, \aap, nov, Volume 535, p.A128, (2011)