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<ri:Resource created="2017-03-10T07:22:14Z" 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>Glycolaldehyde in Perseus young solar analogs</title><shortName>J/A+A/599/A121</shortName><identifier>ivo://CDS.VizieR/J/A+A/599/A121</identifier><altIdentifier>doi:10.26093/cds/vizier.35990121</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De Simone M.</name></creator><creator><name>Codella C.</name></creator><creator><name>Testi L.</name></creator><creator><name>Belloche A.</name></creator><creator><name>Maury A.J.</name></creator><creator><name>Anderl S.,Andre P.</name></creator><creator><name>Maret S.</name></creator><creator><name>Podio L.</name></creator><date role="Updated">2017-05-02T11:35:11Z</date><date role="Created">2017-03-10T07:22:14Z</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>stellar-associations</subject><subject>g-stars</subject><description>The earliest evolutionary stages of low-mass protostars are characterised by the so-called hot-corino stage, when the newly born star heats the surrounding material and enrich the gas chemically. Studying this evolutionary phase of solar protostars may help understand the evolution of prebiotic complex molecules in the development of planetary systems. In this paper we focus on the occurrence of glycolaldehyde (HCOCH_2_OH) in young solar analogs by performing the first homogeneous and unbiased study of this molecule in the Class 0 protostars of the nearby Perseus star forming region. 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