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Ultrafast outflows: Galaxy-scale active galactic nucleus feedback

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dc.contributor.authorWagner, A. Y.
dc.contributor.authorUmemura, M
dc.contributor.authorBicknell, Geoffrey
dc.date.accessioned2015-12-13T22:15:42Z
dc.date.issued2013
dc.date.updated2016-02-24T08:56:50Z
dc.description.abstractWe show, using global three-dimensional grid-based hydrodynamical simulations, that ultrafast outflows (UFOs) from active galactic nuclei (AGNs) result in considerable feedback of energy and momentum into the interstellar medium (ISM) of the host galaxy.
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/1885/70521
dc.publisherInstitute of Physics Publishing Ltd.
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal Letters
dc.subjectKeywords: galaxies: evolution; galaxies: formation; hydrodynamics; ISM: jets and outflows; methods: numerical
dc.titleUltrafast outflows: Galaxy-scale active galactic nucleus feedback
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage5
local.bibliographicCitation.startpage1
local.contributor.affiliationWagner, A. Y., University of Tsukuba
local.contributor.affiliationUmemura, M, University of Tsukuba
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidBicknell, Geoffrey, u8000061
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB2336
local.identifier.citationvolume763
local.identifier.doi10.1088/2041-8205/763/1/L18
local.identifier.scopusID2-s2.0-84872362880
local.identifier.thomsonID000313564500018
local.type.statusPublished Version

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