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<ri:Resource created="2015-12-11T14:13:01Z" 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>CHemical Abundances of Spirals (CHAOS) II. M51</title><shortName>J/ApJ/808/42</shortName><identifier>ivo://CDS.VizieR/J/ApJ/808/42</identifier><altIdentifier>doi:10.26093/cds/vizier.18080042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Croxall K.V.</name></creator><creator><name>Pogge R.W.</name></creator><creator><name>Berg D.A.</name></creator><creator><name>Skillman E.D.</name></creator><creator><name>Moustakas J.</name></creator><date role="Updated">2024-11-18T20:10:42Z</date><date role="Created">2015-12-11T14:13:01Z</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><description>We have observed NGC 5194 (M51a) as part of the CHemical Abundances of Spirals project (CHAOS). Using the Multi Object Double Spectrographs on the Large Binocular Telescope we are able to measure one or more of the temperature-sensitive auroral lines ([OIII]{lambda}4363, [NII]{lambda}5755, [SIII]{lambda}6312) and thus measure "direct" gas-phase abundances in 29 individual HII regions. [OIII]{lambda}4363 is only detected in two HII regions, both of which show indications of excitation by shocks. We compare our data to previous direct abundances measured in NGC 5194 and find excellent agreement ({Delta}[log(O/H)]~0.05) for all but one region. We find no evidence of trends in Ar/O, Ne/O, or S/O within NGC 5194 or compared to other galaxies. We find modest negative gradients in both O/H and N/O with very little scatter ({sigma}&lt;=0.08dex), most of which can be attributed to random error and not to intrinsic dispersion. The gas-phase abundance gradient is consistent with the gradients observed in other interacting galaxies, which tend to be shallower than gradients measured in isolated galaxies. The N/O ratio (&lt;log(N/O)&gt;=-0.62) suggests secondary nitrogen production is responsible for a significantly larger fraction of nitrogen (e.g., factor of 8-10), relative to primary production mechanisms than predicted by theoretical models.</description><source format="bibcode">2015ApJ...808...42C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/808/42</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/J/ApJ/806/16">J/ApJ/806/16 : CHemical Abundances of Spirals (CHAOS) I. NGC628 (Berg+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2316">J/MNRAS/424/2316 : Abundances in HII regions (Pilyugin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/735/75">J/ApJ/735/75 : HST observations of HII regions in M51 (Lee+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/233">J/ApJS/190/233 : Spectroscopy &amp; abundances of SINGS galaxies (Moustakas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/416">J/AJ/140/416 : IR photometry of massive stars in the SMC (Bonanos+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/654">J/ApJ/700/654 : Keck spectroscopy of extragalactic HII regions (Esteban+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/580">J/ApJ/695/580 : Oxygen abundance in M83 (Bresolin+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2563">J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/675/1213">J/ApJ/675/1213 : Abundances in M33 HII regions (Rosolowsky+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2559">J/AJ/133/2559 : Compact radio sources in spiral galaxies. II. (Maddox+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/441/981">J/A+A/441/981 : HII regions in 5 spiral galaxies (Bresolin+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/240">J/ApJ/617/240 : Oxygen abundances in the GOODS-North field (Kobulnicky+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2867">J/AJ/126/2867 : Red supergiants in Magellanic Clouds (Massey+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/424/599">J/ApJ/424/599 : Abundances in barred spiral galaxies (Martin+ 1994)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/808/42</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/808/42</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/808/42</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/808/42</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/808/42</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/808/42</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/808/42/obs (NGC 5194 MODS/LBT observations and equivalent widths (tables 2 and 3b))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/808/42/obs?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/808/42/obs?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/808/42/obs?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>202.470833</ra><dec>47.197806</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/11026-11027</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/808/42?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/808/42/obs</name><description>NGC 5194 MODS/LBT observations and equivalent widths (tables 2 and 3b)</description><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>recno</name><description>Record number assigned by the VizieR team. 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Uncertainty in Te([SIII])1</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ne1</name><description>Measured Electron density (cm^{-3})</description><unit>cm**-3</unit><ucd>phys.density;phys.electron</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Ne1</name><description>Uncertainty in Ne1</description><unit>cm**-3</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Te([OII])2</name><description>Adopted Electron temperature in the [OII] region</description><unit>K</unit><ucd>phys.temperature;phys.electron</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Te([OII])2</name><description>Uncertainty in Te([OII])2</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Te([OIII])2</name><description>Adopted Electron temperature in the [OIII] region</description><unit>K</unit><ucd>phys.temperature;phys.electron</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logO/H</name><description>Oxygen abundance, 12+log(O/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logO/H</name><description>Uncertainty in O/H</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>N+/H+</name><description>Abundance ratio N+/H+</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_N+/H+</name><description>Uncertainty in N+/H+</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ICF(N)</name><description>Nitrogen ionization correction factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ICF(N)</name><description>Uncertainty in ICF(N)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(N/O)</name><description>Nitrogen-to-oxygen abundance ratio, log(N/O)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(N/O)</name><description>Uncertainty in O/H</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(N/H)</name><description>Nitrogen abundance, 12+log(N/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(N/H)</name><description>Uncertainty in N/H</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S+/H+</name><description>Abundance ratio S+/H+</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S+/H+</name><description>Uncertainty in S+/H+</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S++/H+</name><description>Abundance ratio S++/H+</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S++/H+</name><description>Uncertainty in S++/H+</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ICF(S)</name><description>Uncertainty in ICF(S)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(S/O)</name><description>Sulfer-to-oxygen abundance ratio, log(S/O)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(S/O)</name><description>Uncertainty in S/O</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(S/H)</name><description>Sulfer abundance, 12+log(S/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(S/H)</name><description>Uncertainty in S/H</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ne++/H+</name><description>? Abundance ratio Ne++/H+</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ne++/H+</name><description>? Uncertainty in Ne++/H+</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ICF(Ne)</name><description>Neon ionization correction factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ICF(Ne)</name><description>Uncertainty in ICF(Ne)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Ne/O)</name><description>? Neon-to-oxygen abundance ratio, log(Ne/O)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_log(Ne/O)</name><description>? Uncertainty in Ne/O</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>log(Ne/H)</name><description>? Neon abundance, 12+log(Ne/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(Ne/H)</name><description>? Uncertainty in Ne/H</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ar++/H+</name><description>Abundance ratio Ar++/H+</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ar++/H+</name><description>Uncertainty in Ar++/H+</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ICF(Ar)</name><description>Argon ionization correction factor</description><ucd>arith.factor</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_ICF(Ar)</name><description>Uncertainty in ICF(Ar)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Ar/O)</name><description>Argon-to-oxygen abundance ratio, log(Ar/O)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(Ar/O)</name><description>Uncertainty in Ar/O</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Ar/H)</name><description>Argon abundance, 12+log(Ar/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_log(Ar/H)</name><description>Uncertainty in Ar/H</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>