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<ri:Resource created="2021-05-31T16:29:34Z" 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>Polarization of seven MBM clouds stars</title><shortName>J/MNRAS/476/4442</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/476/4442</identifier><altIdentifier>doi:10.26093/cds/vizier.74764442</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neha S.</name></creator><creator><name>Maheswar G.</name></creator><creator><name>Soam A.</name></creator><creator><name>Lee C.W.</name></creator><date role="Updated">2024-08-18T20:18:40Z</date><date role="Created">2021-05-31T16:29:34Z</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 made R-band polarization measurements of 234 stars towards the direction of the MBM 33-39 cloud complex. The distance of the MBM 33-39 complex was determined as 120+/-10pc using polarization results and near-infrared photometry from the 2MASS survey. The magnetic field geometry of the individual clouds inferred from our polarimetric results reveals that the field lines are in general consistent with the global magnetic field geometry of the region obtained from previous studies. This implies that the clouds in the complex are permeated by the interstellar magnetic field. Multi-wavelength polarization measurements of a few stars projected on to the complex suggest that the size of the dust grains in these clouds is similar to those found in the normal interstellar medium of the Milky Way. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster name, MBM 33, MBM 34 and MBM 35</description><ucd>meta.id.parent</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Star</name><description>[1/30] Star ID</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>PV</name><description>Polarisation degree in V band</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PV</name><description>rms uncertainty on PV</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetaV</name><description>Polarisation angle in V band</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_thetaV</name><description>rms uncertainty on thetaV</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PR</name><description>Polarisation degree in R band</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PR</name><description>rms uncertainty on PR</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetaR</name><description>Polarisation angle in R band</description><unit>deg</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_thetaR</name><description>rms uncertainty on thetaR</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PI</name><description>Polarisation degree in I band</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PI</name><description>rms uncertainty on PI</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetaI</name><description>Polarisation angle in I band</description><unit>%</unit><ucd>pos.posAng;phys.polarization</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_thetaI</name><description>rms uncertainty on thetaI</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambdamax</name><description>Wavelenght of maximum degree of polarization</description><unit>%</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_lambdamax</name><description>rms uncertainty on lambdamax</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Pmax</name><description>Maximum degree of polarization as a percentage at wavelength lambdamax</description><unit>um</unit><ucd>phys.polarization;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Pmax</name><description>rms uncertainty on Pmax</description><unit>um</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RV</name><description>Total-to-selective extinction</description><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RV</name><description>rms uncertainty on RV</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/MNRAS/476/4442/table7</name><description>Polarization results of 234 stars observed in the direction of the MBM 33-39 cloud complex with P/{sigma}_P_&gt;=2</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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