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<ri:Resource created="2013-07-23T12:06:43Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>H{alpha} and UV fluxes in nearby galaxies</title><shortName>J/ApJ/744/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/744/44</identifier><altIdentifier>doi:10.26093/cds/vizier.17440044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Weisz D.R.</name></creator><creator><name>Johnson B.D.</name></creator><creator><name>Johnson L.C.</name></creator><creator><name>Skillman E.D.</name></creator><creator><name>Lee J.C.,Kennicutt R.C.</name></creator><creator><name>Calzetti D.</name></creator><creator><name>van Zee L.</name></creator><creator><name>Bothwell M.S.</name></creator><creator><name>Dalcanton J.J.,Dale D.A.</name></creator><creator><name>Williams B.F.</name></creator><date role="Updated">2017-11-06T12:23:40Z</date><date role="Created">2013-07-23T12:06:43Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>ultraviolet-astronomy</subject><subject>surface-photometry</subject><subject>absolute-magnitude</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>We consider the effects of non-constant star formation histories (SFHs) on H{alpha} and GALEX far-ultraviolet (FUV) star formation rate (SFR) indicators. Under the assumption of a fully populated Chabrier initial mass function (IMF), we compare the distribution of H{alpha}-to-FUV flux ratios from ~1500 simple, periodic model SFHs with observations of 185 galaxies from the Spitzer Local Volume Legacy survey. We find a set of SFH models that are well matched to the data, such that more massive galaxies are best characterized by nearly constant SFHs, while low-mass systems experience burst amplitudes of ~30 (i.e., an increase in the SFR by a factor of 30 over the SFR during the inter-burst period), burst durations of tens of Myr, and periods of ~250 Myr; these SFHs are broadly consistent with the increased stochastic star formation expected in systems with lower SFRs. We analyze the predicted temporal evolution of galaxy stellar mass, R-band surface brightness, H{alpha}-derived SFR, and blue luminosity, and find that they provide a reasonable match to observed flux distributions. We find that our model SFHs are generally able to reproduce both the observed systematic decline and increased scatter in H{alpha}-to-FUV ratios toward low-mass systems, without invoking other physical mechanisms.</description><source format="bibcode">2012ApJ...744...44W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/744/44</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/6">J/ApJS/192/6 : A GALEX UV 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