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)
Titre | 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) |
Type de publication | Journal Article |
Year of Publication | 2014 |
Auteurs | Traficante, 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 |
Volume | 440 |
Pagination | 3588-3612 |
Date Published | jun |
Mots-clés | dust, extinction, Galaxy: structure, infrared: ISM |
DOI | 10.1093/mnras/stu493 |
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