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Resolving the coronal line region of NGC 1068 with near-infrared integral field spectroscopy

dc.contributor.authorMazzalay, X
dc.contributor.authorRodriıguez-Ardila, A
dc.contributor.authorKomossa, S
dc.contributor.authorMcGregor, Peter
dc.date.accessioned2015-12-13T22:23:07Z
dc.date.issued2013
dc.date.updated2016-02-24T09:09:26Z
dc.description.abstractWe present adaptive optics-assisted J- and K-band integral field spectroscopy of the inner 300 × 300 pc of the Seyfert 2 galaxy NGC 1068. The data were obtained with the Gemini Near-infrared Integral-Field Spectrograph integral field unit spectrometer, w
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/72605
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Galaxies: active; Galaxies: kinematics and dynamics; Galaxies: nuclei; Infrared: galaxies; Line: formation; Line: profiles
dc.titleResolving the coronal line region of NGC 1068 with near-infrared integral field spectroscopy
dc.typeJournal article
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage2426
local.bibliographicCitation.startpage2411
local.contributor.affiliationMazzalay, X, Max-Planck-Institut fur extraterrestrische
local.contributor.affiliationRodriıguez-Ardila, A, Rua Estados Unidos 154
local.contributor.affiliationKomossa, S, Max Planck Institut for Extraterrestrial Physics
local.contributor.affiliationMcGregor, Peter, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidMcGregor, Peter, u8401248
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB3331
local.identifier.citationvolume430
local.identifier.doi10.1093/mnras/stt064
local.identifier.scopusID2-s2.0-84876816558
local.identifier.thomsonID000319260500069
local.type.statusPublished Version

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