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<ri:Resource created="2014-06-27T16:24:14Z" 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>PAH in extragalactic star-forming complexes</title><shortName>J/MNRAS/431/2006</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/431/2006</identifier><altIdentifier>doi:10.26093/cds/vizier.74312006</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Khramtsova M.S.</name></creator><creator><name>Wiebe D.S.</name></creator><creator><name>Boley P.A.</name></creator><creator><name>Pavlyuchenkov YA.N.</name></creator><date role="Updated">2024-07-21T20:14:37Z</date><date role="Created">2014-06-27T16:24:14Z</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>h-ii-regions</subject><subject>infrared-photometry</subject><description>The abundance of polycyclic aromatic hydrocarbons (PAHs) in low- and high-metallicity galaxies has been widely discussed since the time when detailed infrared data for extragalactic objects were first obtained. On the scales of entire galaxies, a smaller PAH abundance in lower metallicity galaxies is often observed. We study this relationship for star-forming regions in nearby galaxies, for a sample containing more than 200 HII complexes, using spatially resolved observations from the Herschel Space Observatory and Spitzer Space Telescope. We use a model for the dust emission to estimate the physical parameters (PAH abundance, metallicity, ultraviolet radiation field, etc.) of these complexes. The same correlation of PAH abundance with metallicity, as seen for entire galaxies, is apparently preserved at smaller scales, at least when the Kobulnicky and Kewley metallicity calibration is used. We discuss possible reasons for this correlation, noting that traces of less effective PAH formation in low-metallicity asymptotic giant branch stars should be smeared out by radial mixing in galactic discs. Effective destruction by the harder and more intensive ultraviolet field in low-metallicity environments is qualitatively consistent with our data, as the ultraviolet field intensity, derived from the infrared photometry, is indeed smaller in HII complexes with lower metallicity.</description><source format="bibcode">2013MNRAS.431.2006K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/431/2006</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/640/768">J/ApJ/640/768 : IR sources in the NGC 5291 system (Higdon+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/127">J/ApJ/686/127 : Starbursts luminosities based on PAH (Weedman+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/705/885">J/ApJ/705/885 : PAH in galaxies at z~0.1 (O'Dowd+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/507/713">J/A+A/507/713 : Galaxies with strong PAH emission (Haas+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/1965">J/ApJ/701/1965 : Radial dust properties of SINGS galaxies (Munoz-Mateos+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/514/A5">J/A+A/514/A5 : PAH luminous galaxies at z~1 (Takagi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A109">J/A+A/527/A109 : Dust and PAH emission SEDs of disk galaxies (Popescu+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/729/94">J/ApJ/729/94 : IR spectroscopy of PAH in 6-15{mu}m band (Ricca+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/744/20">J/ApJ/744/20 : S^4^MC project: 6 star forming regions PAHs (Sandstrom+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/7">J/ApJS/207/7 : Modeling Galactic extinction with dust and PAH (Mulas+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/65/103">J/PASJ/65/103 : PAH3.3um/IR luminosity for infrared galaxies (Yamada+, 2013)</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/MNRAS/431/2006</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/431/2006</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Gal</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType><flag>primary</flag></column><column><name>PropID</name><description>Spitzer proposal ID</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Prop</name><description>Proposer name</description><ucd>obs.observer</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>MType</name><description>Morphological type</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Nc</name><description>[1/23] Number of complexes</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>Reference(s), in refs.dat file</description><ucd>meta.ref;pos.frame;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Res</name><description>Physical resolution</description><unit>kpc</unit><ucd>pos.angResolution</ucd><dataType xsi:type="vs:VOTableType">float</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>NED</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/MNRAS/431/2006/refs</name><description>References</description><column><name>BibCode</name><description>BibCode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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