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<ri:Resource created="2006-06-04T07:10:47Z" 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>Spectroscopy of Southern warm IR galaxies</title><shortName>J/ApJS/132/37</shortName><identifier>ivo://CDS.VizieR/J/ApJS/132/37</identifier><altIdentifier>doi:10.26093/cds/vizier.21320037</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kewley L.J.</name></creator><creator><name>Heisler C.A.</name></creator><creator><name>Dopita M.A.</name></creator><creator><name>Lumsden S.</name></creator><date role="Updated">2017-12-15T10:55:15Z</date><date role="Created">2006-06-04T07:10:47Z</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>infrared-sources</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>In this paper, we present high-resolution optical spectra and optical classifications from our large sample of 285 warm infrared galaxies 10^8^&lt;L_IR_&lt;10^12.5^L_{sun}_. We have classified these galaxies using new theoretical lines on the standard optical diagnostic diagrams. We use a theoretical extreme mixing line between the starburst and AGN regions to classify LINER galaxies and we define a theoretical boundary separating AGNs from starbursts. 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