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A radio-optical study of resolved star formation in SAMI galaxies

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dc.contributor.authorLeslie, Sarah
dc.contributor.authorKewley, Lisa
dc.contributor.authorSadler, Elaine M
dc.contributor.authorBryant, J.
dc.date.accessioned2015-12-10T23:16:30Z
dc.date.issued2014
dc.date.updated2015-12-10T09:53:36Z
dc.description.abstractWith integral field spectroscopic data from the the Sydney-AAO Multi-object Integralfield spectrograph (SAMI) survey and the VLA, we will study the relationship between star formation (as traced by H innodataalpha emission) and the radio continuum emission within galaxies with the aim of better understanding the intricacies of local scaling relations.
dc.identifier.issn1743-9213
dc.identifier.urihttp://hdl.handle.net/1885/65089
dc.publisherCambridge University Press
dc.sourceInternational Astronomical Union. Proceedings
dc.titleA radio-optical study of resolved star formation in SAMI galaxies
dc.typeJournal article
local.bibliographicCitation.issue309
local.bibliographicCitation.lastpage324
local.bibliographicCitation.startpage324
local.contributor.affiliationLeslie, Sarah, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKewley, Lisa, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSadler, Elaine M, University of Sydney
local.contributor.affiliationBryant, J., University of Sydney
local.contributor.authoruidLeslie, Sarah, u5022102
local.contributor.authoruidKewley, Lisa, u9415124
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationa383154xPUB1050
local.identifier.citationvolume10
local.identifier.doi10.1017/S1743921314010199
local.identifier.scopusID2-s2.0-84922503721
local.type.statusPublished Version

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