Unveiling the nature of Seyfert nuclei with 1 - 100 micron spectral energy distributions

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dc.contributor.author Buchanan, Catherine
dc.contributor.author Gallimore, Jack
dc.contributor.author Dea, Christopher
dc.contributor.author Baum, Stefi
dc.contributor.author Axon, David
dc.contributor.author Robinson, Andrew
dc.contributor.author Noel-Storr, Jacob
dc.contributor.author Yzaguirre, A.
dc.contributor.author Elitzur, Moshe
dc.contributor.author Elvis, Martin
dc.contributor.author Tadhunter, Clive
dc.date.accessioned 2008-09-29T19:27:06Z
dc.date.available 2008-09-29T19:27:06Z
dc.date.issued 2008-07-25
dc.identifier.citation arXiv:0807.3993v1 [astro-ph] en_US
dc.identifier.uri http://hdl.handle.net/1850/7114
dc.description Talk given at "The Central Kiloparsec: Active Galactic Nuclei and Their Hosts", Ierapetra, Crete, 4-6 June, 2008. To appear in Volume 79 of the Memorie della Societa Astronomica Italiana. 4 pages, 5 figures en_US
dc.description.abstract The infrared is a key wavelength regime for probing the dusty, obscured nuclear regions of active galaxies. We present results from an infrared study of 87 nearby Seyfert galaxies using the Spitzer Space Telescope and ground-based telescopes. Combining detailed modelling of the 3 - 100 micron spectral energy distributions with mid-IR spectral diagnostics and near-infrared observations, we find broad support for the unified model of AGNs. The IR emission of Seyfert 1s and 2s is consistent with their having the same type of central engine viewed at a different orientation. The nature of the putative torus is becoming clearer; in particular we present evidence that it is likely a clumpy medium. Midinfrared correlations between tracers of star formation and AGN ionizing luminosity reveal the starburst-AGN connection implied by the black hole/bulge mass relation, however it is not yet clear if this is due to feedback. en_US
dc.language.iso en_US en_US
dc.publisher Memorie della Societa Astronomica Italiana en_US
dc.relation RIT Scholars content from RIT Digital Media Library has moved from http://ritdml.rit.edu/handle/1850/7114 to RIT Scholar Works http://scholarworks.rit.edu/other/247, please update your feeds & links!
dc.relation.ispartofseries vol. 79 en_US
dc.subject Galaxies Seyfert en_US
dc.subject Galaxies active en_US
dc.subject Galaxies stellar content en_US
dc.subject Infrared galaxies en_US
dc.title Unveiling the nature of Seyfert nuclei with 1 - 100 micron spectral energy distributions en_US
dc.type Proceedings en_US

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