id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2428	Sánchez-Portal, M.; Castillo-Fraile, M.; Almeida, C. Ramos; Esquej, P.; Alonso-Herrero, A.; Pérez García, A. M.; Acosta-Pulido, J.; Altieri, B.; Bongiovanni, A.; Castro Céron, J. M.; Cepa, J.; Coia, D.; Conversi, L.; Fritz, J.; Gonzalez-Serrano, J. I.; Hatziminaoglou, E.; Povic, M.; Rodrguez Espinosa, J. M.; Valtchanov, I.	Recent Results from the SAFIR Project	2014	4	.pdf	application/pdf	2956	116	59	The quality of the Her- schel data is allowing us to study the spatial distri- bution of dust within the galaxies, thus permitting to characterize the variation of dust properties (tempera- ture, dust mass) and SFR with the nuclear distance. Therefore, dust thermal emission should be made-up of three different contributions: (a) warm dust heated by the AGN (120-170 K); (b) cold dust heated by the star formation (40-70 K, and (c) very cold dust heated by the general interstellar radiation field (15-25 K).	cache/app01-2428.pdf	txt/app01-2428.txt