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<ri:Resource created="2015-03-17T14:29:21Z" 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>Magnetic field structure around cores with VeLLOs</title><shortName>J/A+A/573/A34</shortName><identifier>ivo://CDS.VizieR/J/A+A/573/A34</identifier><altIdentifier>doi:10.26093/cds/vizier.35730034</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Soam A.</name></creator><creator><name>Maheswar G.</name></creator><creator><name>Lee C.W.</name></creator><creator><name>Dib S.</name></creator><creator><name>Bhatt H.C.</name></creator><creator><name>Tamura M.</name></creator><date role="Updated">2015-08-03T15:33:19Z</date><date role="Created">2015-03-17T14:29:21Z</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>magnetic-fields</subject><subject>polarimetry</subject><description>We carried out optical polarimetry of five dense cores, (IRAM 04191, L1521F, L328, L673-7, and L1014) which are found to harbour very low luminosity objects (VeLLOs; Lint&lt;~0.1L_{sun}_). This study was conducted mainly to understand the role played by the magnetic field in the formation of very low and substellar mass range objects. Light from the stars, while passing through the dust grains that are aligned with their short axis parallel to an external magnetic field, becomes linearly polarised. The polarisation position angles measured for the stars can provide the plane-of-the sky magnetic field orientation. 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