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Abstract: The "Seyfert and star formation Activity in the Far-Infrared" (SAFIR) project is aimed at studying the physical nature of the nuclear IR emission and star formation properties of a small sample of nearby Seyfert galaxies observed with the PACS and SPIRE instruments on board the Herschel space observatory. In this paper, we review the achieved results, that reveal the importance of the far-IR range to improve the quality and reliability of the estimates of basic AGN torus parameters, and describe some preliminary outcome from the on-going work on the dust properties of resolved AGN host galaxies.
Fuente: Acta Polytechnica CTU Proceedings, 2014, 1(1), 307-310
Editorial: Czech Technical University
Año de publicación: 2014
Nº de páginas: 4
Tipo de publicación: Artículo de Revista
DOI: 10.14311/APP.2014.01.0307
ISSN: 2336-5382
Url de la publicación: https://doi.org/10.14311/APP.2014.01.0307
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SÁNCHEZ-PORTAL, M.
CASTILLO FRAILE, M.
RAMOS ALMEIDA, CRISTINA
ESQUEJ, P.
ALMUDENA ALONSO HERRERO
PÉREZ GARCÍA, A. M.
ACOSTA PULIDO, J.
ALTIERI, B.
BONGIOVANNI, A.
CASTRO CERÓN, J. M.
CEPA, JORDI
COIA, D.
CONVERSI, L.
FRITZ, J.
JOSE IGNACIO GONZALEZ SERRANO
HATZIMINAOGLOU, E.
RODRÍGUEZ, ESPINOSA, J. M.
VALTCHANOV, I.
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