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)

TitreThe 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)
Type de publicationJournal Article
Year of Publication2014
AuteursTraficante, A., Paladini R., Compiègne M., Alves M. I. R., Cambrésy L., Gibson S. J., Tibbs C. T., Noriega-Crespo A., Molinari S., Carey S. J., Ingalls J. G., Natoli P., Davies R. D., Davis R. J., Dickinson C., and Fuller G. A.
Journal\mnras
Volume440
Pagination3588-3612
Date Publishedjun
Mots-clésdust, extinction, Galaxy: structure, infrared: ISM
DOI10.1093/mnras/stu493
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