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<ri:Resource created="2025-02-27T12:35:11Z" status="active" updated="2025-08-11T20:18:56Z" 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 study in NGC 2345 direction</title><shortName>J/MNRAS/513/4899</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/513/4899</identifier><altIdentifier>doi:10.26093/cds/vizier.75134899</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Singh S.</name></creator><creator><name>Pandey J.C.</name></creator><creator><name>Hoang T.</name></creator><date role="Updated">2025-08-11T20:18:56Z</date><date role="Created">2025-02-27T12:35:11Z</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>milky-way-galaxy</subject><subject>open-star-clusters</subject><subject>interstellar-medium</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>polarimetry</subject><subject>stellar-associations</subject><subject>astrometry</subject><description>We have investigated the grain alignment and dust properties towards the direction of the cluster NGC 2345 using the multiband optical polarimetric observations. For the majority of the stars, the observed polarization is found to be due to the interstellar medium with average values of maximum polarization and wavelength corresponding to it as 1.55 per cent and 0.58 {mu}m, respectively. This reveals a similar size distribution of dust grains to that in the general interstellar medium in the direction of NGC 2345. Alteration of dust properties near the distance of 1.2 kpc towards the direction of NGC 2345 has been noticed. The dust grains located beyond this distance are found to be aligned with the Galactic magnetic field, whereas a dispersion in the orientation of the dust grains lying in the foreground of this distance is found. Polarizing efficiency of grains in this direction is found to be close to the average efficiency for our Galaxy. The decreased grain size along with the increased polarizing efficiency towards the core region of the cluster indicates the local radiation field is higher within the cluster, which is responsible for the increased alignment efficiency of small grains. The wavelength of maximum polarization (associated with the average size of aligned grains) is also found to increase with extinction and reduces with the increase in polarizing efficiency, which can be explained by the radiative torque alignment mechanism.</description><source format="bibcode">2022MNRAS.513.4899S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/513/4899</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/J/A+A/618/A93">J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/161/149">J/AJ/161/149 : Vilnius photometry in IC 59 and IC 63 (Soam+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/160/256">J/AJ/160/256 : Polarization of 125 stars in NGC 1817 open cluster</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/631/A124">J/A+A/631/A124 : NGC 2345 Stroemgren photometry (Alonso-Santiago+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : Milky Way global survey of star clusters. II.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</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/MNRAS/513/4899</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/513/4899</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/513/4899</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/513/4899</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/513/4899</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/513/4899</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/513/4899/table1 (The degree of polarization P and polarization position angle ({Theta}) in four bands B/V/R/I for observed stars in the cluster NGC 2345 and a field region)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/513/4899/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/513/4899/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/513/4899/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>107.1331039</ra><dec>-13.1699356</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/21632-21633 21635</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/513/4899?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/513/4899/table1</name><description>The degree of polarization P and polarization position angle ({Theta}) in four bands B/V/R/I for observed stars in the cluster NGC 2345 and a field region</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>Region</name><description>Region Cluster or Field region</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>ID</name><description>Identifier number (ID)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_ID</name><description>ID marked with asterisk symbol are members of the cluster NGC 2345</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>GaiaDR2</name><description>Gaia DR2 source identifier (Gaia)</description><ucd>meta.id;meta.main</ucd></column><column><name>Offset</name><description>Offset position between ARIES and Gaia positions (Offset)</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PB</name><description>? Degree of polarization in the B band (P_B_)</description><unit>%</unit><ucd>phys.polarization;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PB</name><description>? Mean error of P_B_ (errorP_B_)</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PAB</name><description>? Position angle of polarization in the B band ({Theta}_B_)</description><unit>deg</unit><ucd>pos.posAng;phys.polarization;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PAB</name><description>? Mean error of PAB (error{Theta}_B_)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PV</name><description>? Degree of polarization in the V band (P_V_)</description><unit>%</unit><ucd>phys.polarization;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PV</name><description>? Mean error of P_V_ (errorP_V_)</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PAV</name><description>? Position angle of polarization in the V band ({Theta}_V_)</description><unit>deg</unit><ucd>pos.posAng;phys.polarization;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PAV</name><description>? Mean error of PAV ( (error{Theta}_V_)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PR</name><description>? Degree of polarization in the R band (P_R_)</description><unit>%</unit><ucd>phys.polarization;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PR</name><description>? Mean error of P_R_ (errorP_R_)</description><unit>%</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PAR</name><description>? Position angle of polarization in the R band ({Theta}_R_)</description><unit>deg</unit><ucd>pos.posAng;phys.polarization;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_PAR</name><description>? Mean error of PAR (error{Theta}_R_)</description><unit>deg</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>PI</name><description>? 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