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Theoretical evolution of optical strong lines across cosmic time

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dc.contributor.authorKewley, Lisa
dc.contributor.authorDopita, Michael
dc.contributor.authorLeitherer, Claus
dc.contributor.authorDave, Romeel
dc.contributor.authorYuan, T.-T.
dc.contributor.authorAllen, Mark G.
dc.contributor.authorGroves, Brent A
dc.contributor.authorSutherland, Ralph
dc.date.accessioned2015-12-13T22:27:12Z
dc.date.issued2013
dc.date.updated2015-12-11T08:29:21Z
dc.description.abstractWe use the chemical evolution predictions of cosmological hydrodynamic simulations with our latest theoretical stellar population synthesis, photoionization, and shock models to predict the strong line evolution of ensembles of galaxies from z = 3 to the
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/73839
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.titleTheoretical evolution of optical strong lines across cosmic time
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage17
local.bibliographicCitation.startpage1
local.contributor.affiliationKewley, Lisa, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLeitherer, Claus, Space Telescope Science Institute
local.contributor.affiliationDave, Romeel, University of the Western Cape
local.contributor.affiliationYuan, T.-T., University of Hawaii
local.contributor.affiliationAllen, Mark G., Observatoire de Strasbourg
local.contributor.affiliationGroves, Brent A, Max Planck Institute for Astrophysics
local.contributor.affiliationSutherland, Ralph, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidKewley, Lisa, u9415124
local.contributor.authoruidDopita, Michael, u7501303
local.contributor.authoruidSutherland, Ralph, u8517070
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB3854
local.identifier.ariespublicationu4630950xPUB180
local.identifier.citationvolume774
local.identifier.doi10.1088/0004-637X/774/2/100
local.identifier.scopusID2-s2.0-84883632736
local.identifier.thomsonID000323888900009
local.type.statusPublished Version

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