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<ri:Resource created="2021-02-24T10:15:36Z" 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>SFR &amp; gas-phase metallicity in MaNGA gal.</title><shortName>J/ApJ/882/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/882/9</identifier><altIdentifier>doi:10.26093/cds/vizier.18820009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanchez-Menguiano L.</name></creator><creator><name>Sanchez Almeida J.</name></creator><creator><name>Munoz-Tunon C.</name></creator><creator><name>Sanchez S.F.,Filho M.</name></creator><creator><name>Hwang H.-C.</name></creator><creator><name>Drory N.</name></creator><date role="Updated">2021-09-10T14:11:33Z</date><date role="Created">2021-02-24T10:15:36Z</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>chemical-abundances</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>galaxy-kinematics</subject><subject>galaxy-classification-systems</subject><subject>surveys</subject><description>The role of gas accretion in galaxy evolution is still a matter of debate. The presence of inflows of metal-poor gas that trigger star formation bursts of low metallicity has been proposed as an explanation for the local anticorrelation between star formation rate (SFR) and gas-phase metallicity (Z_g_) found in the literature. In the present study, we show how the anticorrelation is also present as part of a diversified range of behaviors for a sample of more than 700 nearby spiral galaxies from the SDSS-IV MaNGA survey. We have characterized the local relation between SFR and Z_g_ after subtracting the azimuthally averaged radial profiles of both quantities. Of the analyzed galaxies, 60% display an SFR-Z_g_ anticorrelation, with the remaining 40% showing no correlation (19%) or positive correlation (21%). Applying a random forest machine-learning algorithm, we find that the slope of the correlation is mainly determined by the average gas-phase metallicity of the galaxy. Galaxy mass, g-r colors, stellar age, and mass density seem to play a less significant role. This result is supported by the performed second-order polynomial regression analysis. Thus, the local SFR-Z_g_ slope varies with the average metallicity, with the more metal-poor galaxies presenting the lowest slopes (i.e., the strongest SFR-Z_g_ anticorrelations), and reversing the relation for more metal-rich systems. Our results suggest that external gas accretion fuels star formation in metal-poor galaxies, whereas in metal-rich systems, the gas comes from previous star formation episodes.</description><source format="bibcode">2019ApJ...882....9S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/882/9</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/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/259">J/ApJ/695/259 : Massive metal-poor galaxies from SDSS (Peeples+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/414/2602">J/MNRAS/414/2602 : Automated classification of HIP variables (Dubath+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A114">J/A+A/559/A114 : Updated O3N2 and N2 abundance indicators (Marino+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A70">J/A+A/587/A70 : CALIFA face-on spiral galaxies (Sanchez-Menguiano+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/86">J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/2570">J/MNRAS/466/2570 : Low ionization emission-line regions (Belfiore+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A122">J/A+A/623/A122 : Sample of MaNGA galaxies properties (Pilyugin+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A171">J/A+A/623/A171 : Mkn 848 MaNGA 3-D data cube 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Average LW stellar metallicity at disk effective radius</description><unit>log(Sun)</unit><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sigma0</name><description>[0/280] Central stellar velocity dispersion</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]</name><description>[-0.4/0.5]? Slope of the oxygen abundance gradient</description><ucd>arith.grad;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sSFR</name><description>[-2.8/1.2] Specific star formation rate</description><unit>log(Gyr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SFR-Zg</name><description>[-0.2/0.11] Slope of the local SFR-Z_g_ relation</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SFR-Zg</name><description>[0.001/0.4] SFR-Zg uncertainty</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sloan</name><description>Display the online SDSS-DR15 online data for the nearest object</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from MaNGA DR15 (Wake+, 2017, J/AJ/154/86) (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from MaNGA DR15 (Wake+, 2017, J/AJ/154/86) (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>