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<ri:Resource created="2021-03-04T07:07:45Z" 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 125 stars in NGC 1817 open cluster</title><shortName>J/AJ/160/256</shortName><identifier>ivo://CDS.VizieR/J/AJ/160/256</identifier><altIdentifier>doi:10.26093/cds/vizier.51600256</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Singh S.</name></creator><creator><name>Pandey J.C.</name></creator><date role="Updated">2021-07-05T09:03:46Z</date><date role="Created">2021-03-04T07:07:45Z</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>interstellar-medium</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>polarimetry</subject><description>Multiband linear polarimetric observations of 125 stars in the region of the cluster NGC1817 have been carried out intending to study properties of interstellar dust and grains in that direction. The polarization is found to be wavelength-dependent, being maximum in the V-band with an average value of 0.95%. The foreground interstellar dust grains appear to be the main source of linear polarization of starlight toward the direction of NGC1817. The average value of the position angle in the V-band of 119.2{deg} is found to be less than the direction of the Galactic parallel in the region, indicating that the dust grains in the direction are probably not yet relaxed. Spatial distribution of dust appears to be more diverse in the coronal region than the core region of the cluster. The maximum value of the degree of polarization is estimated to be 0.93% for members of the cluster using the Serkowski relation. The average value of wavelength corresponding to the maximum polarization of 0.54{+/-}0.02{mu}m indicates that the size distribution of dust grains in the line of sight is similar to that of the general interstellar medium. Several variable stars in the cluster were also observed polarimetrically and pulsating variables appear to have a slightly lower value of polarization from other nonvariable member stars of the cluster. There are indications of the existence of dust layers in front of those clusters which are located close to galactic plane while for clusters located away from galactic plane no major dust layers are observed.</description><source format="bibcode">2020AJ....160..256S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/256</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/178">II/178 : Linear polarization measurements for 5070 stars (Axon+ 1976)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/226">II/226 : Stellar polarization catalogs agglomeration (Heiles, 2000)</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><relatedResource ivo-id="ivo://CDS.VizieR/I/349">I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+,2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/96">V/96 : Catalogue of open cluster parameters from UBV-data.(Loktin+, 1994)</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/J/ApJS/2/389">J/ApJS/2/389 : Observations of O and B stars (Hiltner, 1956)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/359/347">J/A+A/359/347 : Reddening in open and globular clusters (Dutra+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/426/819">J/A+A/426/819 : NGC1817 proper motions and membership (Balaguer-Nunez+,2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/438/1163">J/A+A/438/1163 : Catalogue of Open Cluster Data (COCD) (Kharchenko+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/463/789">J/A+A/463/789 : Blue stragglers in open clusters (Ahumada+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/462/621">J/A+A/462/621 : UBVRI polarisation in NGC 5749 (Vergne+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/2146">J/MNRAS/399/2146 : Orbits of open clusters in the Galaxy (Wu+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/403/1577">J/MNRAS/403/1577 : Polarization towards open cluster NGC 6823 (Medhi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/513/A75">J/A+A/513/A75 : Polarimetry of stars in NGC 5617 (Orsatti+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/522/A88">J/A+A/522/A88 : Photometric identification of BHB stars (Smith+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/403/2041">J/MNRAS/403/2041 : Optical polarization in NGC 6124 (Vergne+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/63/S1">J/PASJ/63/S1 : Atlas &amp; 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