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The pan-spectral energy distribution of dusty narrow line regions

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dc.contributor.authorGroves, Brent
dc.contributor.authorDopita, Michael
dc.contributor.authorSutherland, Ralph
dc.date.accessioned2015-12-13T22:52:03Z
dc.date.available2015-12-13T22:52:03Z
dc.date.issued2005
dc.date.updated2015-12-11T10:48:52Z
dc.description.abstractNarrow line regions (NLR) are a major component of active galaxies, and commonly used as an indicator of the presence of an active galactic nucleus (AGN). Most of the analysis and theoretical work into NLRs so far has concentrated only on the narrow emission lines. However, NLRs show strong evidence of containing dust and will likely emit strongly in the infrared. Here, we model this radiation from NLRs, examining the effects of pressure and ionization parameter, and demonstrate that a large fraction of the NLR emission is emerges in the IR.
dc.identifier.isbn0735402469
dc.identifier.urihttp://hdl.handle.net/1885/81381
dc.publisherAmerican Institute of Physics (AIP)
dc.relation.ispartofThe Spectral Energy Distributions of Gas-Rich Galaxies: Confronting Models with Data.
dc.relation.isversionof1st Edition
dc.titleThe pan-spectral energy distribution of dusty narrow line regions
dc.typeBook chapter
local.bibliographicCitation.lastpage276
local.bibliographicCitation.placeofpublicationMelville, NY
local.bibliographicCitation.startpage273
local.contributor.affiliationGroves, Brent Allan, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSutherland, Ralph, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidGroves, Brent Allan, u9816125
local.contributor.authoruidDopita, Michael, u7501303
local.contributor.authoruidSutherland, Ralph, u8517070
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub9683
local.identifier.doi10.1063/1.1913939
local.identifier.scopusID2-s2.0-33645295571
local.type.statusPublished Version

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