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<ri:Resource created="2015-11-10T15:16:55Z" 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>Optical polarimetric catalog of stars in the SMC</title><shortName>J/ApJ/806/94</shortName><identifier>ivo://CDS.VizieR/J/ApJ/806/94</identifier><altIdentifier>doi:10.26093/cds/vizier.18060094</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gomes A.L.</name></creator><creator><name>Magalhaes A.M.</name></creator><creator><name>Pereyra A.</name></creator><creator><name>Rodrigues C.V.</name></creator><date role="Updated">2018-01-30T07:17:50Z</date><date role="Created">2015-11-10T15:16:55Z</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>magellanic-clouds</subject><subject>polarimetry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We present a new optical polarimetric catalog for the Small Magellanic Cloud (SMC). It contains a total of 7207 stars, located in the northeast (NE) and Wing sections of the SMC and part of the Magellanic Bridge. This new catalog is a significant improvement compared to previous polarimetric catalogs for the SMC. We used it to study the sky-projected interstellar magnetic field structure of the SMC. Three trends were observed for the ordered magnetic field direction at position angles (PAs) of (65{deg}+/-10{deg}), (115{deg}+/-10{deg}), and (150{deg}+/-10{deg}). Our results suggest the existence of an ordered magnetic field aligned with the Magellanic Bridge direction and SMC's Bar in the NE region, which have PAs roughly at 115.4{deg} and 45{deg}, respectively. However, the overall magnetic field structure is fairly complex. The trends at 115{deg} and 150{deg} may be correlated with the SMC's bimodal structure, observed in Cepheids' distances and HI velocities. We derived a value of B_sky_=(0.497+/-0.079){mu}G for the ordered sky-projected magnetic field, and {delta}B=(1.465+/-0.069){mu}G for the turbulent magnetic field. This estimate of B_sky_ is significantly larger (by a factor of ~10) than the line of sight field derived from Faraday rotation observations, suggesting that most of the ordered field component is on the plane of the sky. A turbulent magnetic field stronger than the ordered field agrees with observed estimates for other irregular and spiral galaxies. For the SMC the B_sky_/{delta}B ratio is closer to what is observed for our Galaxy than other irregular dwarf galaxies.</description><source format="bibcode">2015ApJ...806...94G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/806/94</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/236">II/236 : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/226">II/226 : Stellar polarization catalogs agglomeration (Heiles, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/1663">J/MNRAS/442/1663 : Velocities of red giants in the SMC (Dobbie+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/698/2031">J/ApJ/698/2031 : Polarimetry of HAeBe stars (Rodrigues+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/688/1029">J/ApJ/688/1029 : Magnetic field in the SMC (Mao+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/91/171">J/A+AS/91/171 : Blue stars between Magellanic Clouds (Demers+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/30/261">J/A+AS/30/261 : UBV and Radial Velocities of SMC Supergiants (Ardeberg+, 1977)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/806/94</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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