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The H Alpha and Infrared Star Formation Rates for the Nearby Field Galaxy Survey

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dc.contributor.authorKewley, Lisa
dc.contributor.authorGellerstedt, Goran
dc.contributor.authorJansen, R A
dc.contributor.authorDopita, Michael
dc.date.accessioned2015-12-13T22:31:00Z
dc.date.available2015-12-13T22:31:00Z
dc.date.issued2002
dc.date.updated2015-12-11T08:58:28Z
dc.description.abstractWe investigate the Ha and infrared star formation rate (SFR) diagnostics for galaxies in the Nearby Field Galaxy Survey (NFGS). For the 81 galaxies in our sample, we derive Hα fluxes (included here) from integrated spectra. There is a strong correlation
dc.identifier.issn0004-6256
dc.identifier.urihttp://hdl.handle.net/1885/75104
dc.publisherUniversity of Chicago Press
dc.sourceAstronomical Journal
dc.subjectKeywords: Dust, extinction; Galaxies: spiral; Galaxies: starburst
dc.titleThe H Alpha and Infrared Star Formation Rates for the Nearby Field Galaxy Survey
dc.typeJournal article
local.bibliographicCitation.lastpage3143
local.bibliographicCitation.startpage3135
local.contributor.affiliationKewley, Lisa J, University of Hawaii
local.contributor.affiliationGellerstedt, Goran, Royal Institute of Technology
local.contributor.affiliationJansen, R A, Arizona State University
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidDopita, Michael, u7501303
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub4468
local.identifier.citationvolume124
local.identifier.doi10.1086/344487
local.identifier.scopusID2-s2.0-0042162677
local.type.statusPublished Version

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