Biblio
4 resultats trouvés
Filtres: Mot-clé is infrared: ISM and Auteur is Molinari, S. [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)
Detection and characterization of a 500 {$μ$}m dust emissivity excess in the Galactic plane using Herschel/Hi-GAL observations,
, \aap, jan, Volume 537, p.A113, (2012)
Dust in the Diffuse Emission of the Galactic Plane: The Herschel/Spitzer Spectral Energy Distribution Fitting,
, \apjl, nov, Volume 724, p.L44-L47, (2010)
Dust temperature tracing the ISRF intensity in the Galaxy,
, \aap, jul, Volume 518, p.L88, (2010)