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<ri:Resource created="2023-10-30T14:14:11Z" 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>H-band polarization around YSOs &amp; BDs</title><shortName>J/ApJ/926/67</shortName><identifier>ivo://CDS.VizieR/J/ApJ/926/67</identifier><altIdentifier>doi:10.26093/cds/vizier.19260067</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Clemens D.P.</name></creator><creator><name>Pillai T.G.S.</name></creator><creator><name>Rilinger A.M.</name></creator><creator><name>Espaillat C.C.</name></creator><date role="Updated">2024-02-14T07:17:02Z</date><date role="Created">2023-10-30T14:14:11Z</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>brown-dwarfs</subject><subject>young-stellar-objects</subject><subject>polarimetry</subject><subject>infrared-sources</subject><description>Wide-field near-infrared (NIR) polarimetry was used to examine disk systems around two brown dwarfs (BDs) and two young stellar objects (YSOs) embedded in the Heiles Cloud 2 (HCl2) dark molecular cloud in Taurus as well as numerous stars located behind HCl2. Inclined disks exhibit intrinsic NIR polarization due to scattering of photospheric light, which is detectable even for unresolved systems. After removing polarization contributions from magnetically aligned dust in HCl2 determined from the background star information, significant intrinsic polarization was detected from the disk systems of one BD (ITG 17) and both YSOs (ITG 15, ITG 25), but not from the other BD (2M0444). The ITG 17 BD shows good agreement of the disk orientation inferred from the NIR and from published Atacama Large Millimeter/submillimeter Array (ALMA) dust continuum imaging. ITG 17 was also found to reside in a 5200 au wide binary (or hierarchical quad star system) with the ITG 15 YSO disk system. The inferred disk orientations from the NIR for ITG 15 and ITG 17 are parallel to each other and perpendicular to the local magnetic field direction. The multiplicity of the system and the large BD disk nature could have resulted from formation in an environment characterized by misalignment of the magnetic field and the protostellar disks.</description><source format="bibcode">2022ApJ...926...67C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/926/67</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/244">VII/244 : Atlas and Catalog of Dark Clouds (Dobashi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IV/34">IV/34 : K2 Ecliptic Plane Input Catalog (EPIC) (Huber+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/350">I/350 : Gaia EDR3 (Gaia Collaboration, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/111">J/ApJS/186/111 : Spitzer observations of Taurus members (Luhman+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/741/21">J/ApJ/741/21 : Polarization of stars in Taurus (Chapman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/129">J/ApJ/771/129 : Submillimetric Class II sources of Taurus (Andrews+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A29">J/A+A/570/A29 : TBOSS Survey I: Herschel/PACS (Bulger+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/578/L6">J/A+A/578/L6 : Polarized images of MWC758 (Benisty+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/176">J/ApJ/833/176 : The magnetic field of L1544. 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