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<ri:Resource created="2012-06-25T11:25:43Z" status="active" updated="2025-06-13T15:25:00Z" 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>Type Ibc SNe in disturbed galaxies</title><shortName>J/ApJ/717/342</shortName><identifier>ivo://CDS.VizieR/J/ApJ/717/342</identifier><altIdentifier>doi:10.26093/cds/vizier.17170342</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Habergham S.M.</name></creator><creator><name>Anderson J.P.</name></creator><creator><name>James P.A.</name></creator><date role="Updated">2017-06-26T11:49:00Z</date><date role="Created">2012-06-25T11:25:43Z</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>supernovae</subject><subject>galaxies</subject><subject>visible-astronomy</subject><subject>h-alpha-photometry</subject><description>We compare the radial locations of 178 core-collapse supernovae (CCSNe) to the R-band and H{alpha} light distributions of their host galaxies. When the galaxies are split into "disturbed" and "undisturbed" categories, a striking difference emerges. The disturbed galaxies have a central excess of CCSNe and this excess is almost completely dominated by supernovae of types Ib, Ic, and Ib/c, whereas type II supernovae dominate in all other environments. The difference cannot easily be explained by metallicity or extinction effects, and thus we propose that this is direct evidence for a stellar initial mass function that is strongly weighted toward high-mass stars, specifically in the central regions of disturbed galaxies.</description><source format="bibcode">2010ApJ...717..342H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/717/342</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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource 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ivo-id="ivo://CDS.VizieR/J/MNRAS/372/1315">J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/115/1280">J/PASP/115/1280 : Classifications of SN host galaxies (van den Bergh+, 2003)</relatedResource><relatedResource>http://www.cbat.eps.harvard.edu/lists/Supernovae.html : IAU list of SNe</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/717/342</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/717/342</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/717/342</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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