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<ri:Resource created="2019-02-11T13:17:50Z" status="active" updated="2026-03-17T20:07:50Z" 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>Fundamental parameters of CP stars</title><shortName>J/other/AstBu/74</shortName><identifier>ivo://CDS.VizieR/J/other/AstBu/74.62</identifier><altIdentifier>doi:10.26093/cds/vizier/dv/hekgc</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Moiseeva A.V.</name></creator><creator><name>Romanyuk I.I.</name></creator><creator><name>Semenko E.A.</name></creator><creator><name>Kudryavtsev D.O.</name></creator><creator><name>Yakunin I.A.</name></creator><date role="Updated">2026-03-17T20:07:50Z</date><date role="Created">2019-02-11T13:17:50Z</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>effective-temperature</subject><subject>optical-observation</subject><subject>catalogs</subject><subject>astronomical-models</subject><subject>stellar-atmospheres</subject><subject>radial-velocity</subject><subject>spectroscopy</subject><subject>peculiar-variable-stars</subject><description>The paper presents the results of determination of fundamental parameters (effective temperature, surface gravity, luminosity, mass, radius, rotation velocity, and radial velocity) for 146 stars observed at the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences with the Main Stellar Spectrograph during 2009-2011; 124 of the stars are magnetic or potentially magnetic objects. We obtained and analyzed at least 500 pairs of circularly-polarized-emission spectra. 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