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<ri:Resource created="2017-11-17T13:18:20Z" 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>N/O ratio of dwarf galaxies from SDSS</title><shortName>J/ApJ/837/42</shortName><identifier>ivo://CDS.VizieR/J/ApJ/837/42</identifier><altIdentifier>doi:10.26093/cds/vizier.18370042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Douglass K.A.</name></creator><creator><name>Vogeley M.S.</name></creator><date role="Updated">2020-01-29T13:50:24Z</date><date role="Created">2017-11-17T13:18:20Z</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>redshifted</subject><subject>absolute-magnitude</subject><description>We examine how the cosmic environment affects the chemical evolution of galaxies in the universe by comparing the N/O ratio of dwarf galaxies in voids with that of dwarf galaxies in denser regions. Ratios of the forbidden [OIII] and [SII] transitions provide estimates of a region's electron temperature and number density. We estimate the abundances of oxygen and nitrogen using these temperature and density estimates and the emission-line fluxes [OII]3727, [OIII]4959,5007, and [NII]6548,6584 with the direct T_e_ method. Using spectroscopic observations from the Sloan Digital Sky Survey Data Release 7, we are able to estimate the N/O ratio in 42 void dwarf galaxies and 89 dwarf galaxies in denser regions. The N/O ratio for void dwarfs (M_r_&gt;-17) is slightly lower (~12%) than for dwarf galaxies in denser regions. We also estimate the nitrogen and oxygen abundances of 2050 void galaxies and 3883 galaxies in denser regions with M_r_&gt;-20. These somewhat brighter galaxies (but still fainter than L_*_) also display similar minor shifts in the N/O ratio. The shifts in the average and median element abundance values in all absolute magnitude bins studied are in the same direction, suggesting that the large-scale environment may influence the chemical evolution of galaxies. We discuss possible causes of such a large-scale environmental dependence of the chemical evolution of galaxies, including retarded star formation and a higher ratio of dark matter halo mass to stellar mass in void galaxies.</description><source format="bibcode">2017ApJ...837...42D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/837/42</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/V/147">V/147 : The SDSS Photometric Catalog, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/511/639">J/ApJ/511/639 : Abundances in blue compact galaxies (Izotov+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/330/75">J/MNRAS/330/75 : Chemical abundances in UV-selected galaxies (Contini+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/448/955">J/A+A/448/955 : Abundances of emission galaxies in SDSS-DR3 (Izotov+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/636/214">J/ApJ/636/214 : HII regions in dwarf irregular galaxies (van Zee+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/140">J/ApJ/765/140 : Stacked spectra of SDSS star forming galaxies (Andrews+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/186">J/ApJ/834/186 : Metallicity of MPA-JHU SDSS-DR7 dwarf gal. 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