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<ri:Resource created="2013-12-06T09:35:41Z" 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>Horsehead H2CO and CH3OH 30m and PdBI maps</title><shortName>J/A+A/560/A73</shortName><identifier>ivo://CDS.VizieR/J/A+A/560/A73</identifier><altIdentifier>doi:10.26093/cds/vizier.35600073</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Guzman V.</name></creator><creator><name>Goicoechea J.R.</name></creator><creator><name>Pety J.</name></creator><creator><name>Gratier P.</name></creator><creator><name>Gerin M.</name></creator><creator><name>Roueff E.,Le Petit F.</name></creator><creator><name>Le Bourlot J.</name></creator><creator><name>Faure A.</name></creator><date role="Updated">2019-03-21T05:37:04Z</date><date role="Created">2013-12-06T09:35:41Z</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>molecular-clouds</subject><subject>radio-astronomy</subject><description>Theoretical models and laboratory experiments show that CH_3_OH is efficiently formed on cold grain surfaces through the successive hydrogenation of CO, forming HCO and H_2_CO as intermediate species. In cold cores and low UV-field illumination photo-dissociation regions (PDRs) the ices can be released into the gas-phase through nonthermal processes such as photodesorption, which considerably increases their gas-phase abundances. 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