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<ri:Resource created="2016-04-20T11:54:00Z" 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>CO, SO and H_2_CO images of AB Aur</title><shortName>J/A+A/589/A60</shortName><identifier>ivo://CDS.VizieR/J/A+A/589/A60</identifier><altIdentifier>doi:10.26093/cds/vizier.35890060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pacheco-Vazquez S.</name></creator><creator><name>Fuente A.</name></creator><creator><name>Baruteau C.</name></creator><creator><name>Berne O.</name></creator><creator><name>Agundez M.</name></creator><creator><name>Neri R.,Goicoechea J.R.</name></creator><creator><name>Cernicharo J.</name></creator><creator><name>Bachiller R.</name></creator><date role="Updated">2016-04-20T10:54:37Z</date><date role="Created">2016-04-20T11:54:00Z</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>pre-main-sequence-stars</subject><subject>radio-astronomy</subject><subject>interferometry</subject><description>Transitional disks are structures of dust and gas around young stars with large inner cavities in which planet formation may occur. Lopsided dust distributions are observed in the dust continuum emission at millimeter wavelengths. These asymmetrical structures can be explained as being the result of an enhanced gas density vortex where the dust is trapped, potentially promoting the rapid growth to the planetesimal scale. AB Aur hosts a transitional disk with a clear horseshoe morphology which strongly suggests the presence of a dust trap. Our goal is to investigate its formation and the possible effects on the gas chemistry. 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