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<ri:Resource created="2003-11-20T19:16:11Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>UBVRI polarization in Stock 16</title><shortName>J/A+A/409/933</shortName><identifier>ivo://CDS.VizieR/J/A+A/409/933</identifier><altIdentifier>doi:10.26093/cds/vizier.34090933</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Feinstein C.</name></creator><creator><name>Baume G.</name></creator><creator><name>Vergne M.M.</name></creator><creator><name>Vazquez R.A.</name></creator><date role="Updated">2003-11-20T18:16:40Z</date><date role="Created">2003-11-20T19:16:11Z</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>open-star-clusters</subject><subject>polarimetry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We present (UBVRI) multicolor linear polarimetric data for 26 of the brightest stars in the area of the open cluster Stock 16 that were considered to study the properties of the ISM (interstellar medium) towards the cluster. Our data yield a mean polarization percentage of P~2.5%, close to the polarization value produced by the ISM with normal efficiency (P_{lambda}_max_~5E_B-V_) undergoing a color excess of E_B-V_=0.51. The mean angle of the polarization vectors, {theta}=74.9deg, agrees quite well with the expected angle produced by dust particles aligned in the direction of the galactic disk (and the magnetic field) in the region. A study of the extinction suffered by the stars in the zone was also performed combining our new data with previous photometric data. In this sense, our analysis indicates that the visual absorption affecting Stock 16 stars is mainly produced in front of the cluster by a dust cloud at approximately 500 pc from the sun. 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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>Name</name><description>Star name (Star NNN, Star WR NN, Star A)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>e_Pol</name><description>rms uncertainty on Pol</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>theta</name><description>Position angle (North to East)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_theta</name><description>rms uncertainty on theta</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SIMBAD</name><description>Designation of star in SIMBAD</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column></table><table><name>J/A+A/409/933/table2</name><description>Parameters of the Serkowski fit to the linear polarization data for stars in Stock 16</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name (Star NNN, Star WR NN, Star A)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Pmax</name><description>Maximum interstellar linear polarisation percentage</description><unit>%</unit><ucd>phys.polarization</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Pmax</name><description>rms uncertainty on Pmax</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigma1</name><description>Unit weight error of the fit (1)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>lambdamax</name><description>Wavelength at which the maximum interstellar linear polarisation occurs, {lambda}_max_</description><unit>um</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>um</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>epsilon</name><description>Dispersion of the position angle normalized by the average of the position angle errors</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SIMBAD</name><description>Designation of star in SIMBAD</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column></table></schema></tableset></ri:Resource>