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机译:Dust temperature tracing the ISRF intensity in the Galaxy
Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, ON M5S 3H8, Canada;
Spitzer Science Center, California Institute of Technology, CALTECH, 1200 East California Boulevard, Pasadena, CA 91125, United States;
Laboratoire d'Astrophysique de Marseille, UMR 6110 CNRS, Université de Provence, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13, FranceJeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, United KingdomMax Planck Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, GermanyRutherford Appleton Laboratory, Chilton, Didcot OX11 0NL, United KingdomINAF, IFSI, via Fosso del Cavaliere 100, Rome, ItalyUniversité de Toulouse, UPS, CESR, 9 avenue du colonel Roche, 31028 Toulouse Cedex 4, FranceInstitut d'Astrophysique Spatiale, Université Paris XI, 91405 Orsay, FranceDipartimento di Fisica, Università di Roma, 1 La Sapienza, Roma, ItalyUniversity of Exeter, Physics Building, Stocker Road, Exeter EX4 4QL, United Kingdom;
dust; extinction; galaxies: ISM; infrared: ISM; ISM: clouds; ISM: general; submillimeter: ISM;