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<ri:Resource created="2014-04-15T08:52:49Z" 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>Galactic plane dust temperature maps with Herschel</title><shortName>J/A+A/564/A111</shortName><identifier>ivo://CDS.VizieR/J/A+A/564/A111</identifier><altIdentifier>doi:10.26093/cds/vizier.35640111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhu J.</name></creator><creator><name>Huang M.</name></creator><date role="Updated">2014-10-09T08:42:17Z</date><date role="Created">2014-04-15T08:52:49Z</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>spectral-energy-distribution</subject><subject>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>Dust grains absorb the interstellar far ultra-violet and visible photons and re-emit them in far-infrared (FIR) wavebands. The dust FIR continuum can be predicted by a grid of models using various values of the interstellar radiation field. We analyze the dust continuum emission in two Hi-GAL science-demonstration phase (SDP) fields using both the radiative transfer code, Cloudy, and the DustEM dust model, to explore the effect of radiative transfer on dust temperature. 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