Recent Results from the SAFIR Project
Typ dokumentu
articlePeer-reviewed
publishedVersion
Autor
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.
Práva
Creative Commons Attribution 4.0 International Licensehttp://creativecommons.org/licenses/by/4.0/
openAccess
Metadata
Zobrazit celý záznamAbstrakt
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.
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