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<ri:Resource created="2017-06-19T15:49:11Z" 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>Rotational properties of mCP stars</title><shortName>J/MNRAS/468/2745</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/468/2745</identifier><altIdentifier>doi:10.26093/cds/vizier.74682745</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Netopil M.</name></creator><date role="Updated">2024-08-17T20:18:39Z</date><date role="Created">2017-06-19T15:49:11Z</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>peculiar-variable-stars</subject><subject>variable-stars</subject><subject>effective-temperature</subject><description>The magnetic chemically peculiar (mCP) stars of the upper main sequence exhibit strong, globally organized magnetic fields that are inclined to the rotational axis and facilitate the development of surface abundance inhomogeneities resulting in photometric and spectroscopic variability. Therefore, mCP stars are perfectly suited for a direct measurement of the rotational period without the need for any additional calibrations. We have investigated the rotational properties of mCP stars based on an unprecedentedly large sample consisting of more than 500 objects with known rotational periods. Using precise parallaxes from the Hipparcos and Gaia satellite missions, well-established photometric calibrations and state-of-the-art evolutionary models, we have determined the location of our sample stars in the Hertzsprung-Russell diagram and derived astrophysical parameters such as stellar masses, effective temperature, radii, inclinations and critical rotational velocities. We have confirmed the conservation of angular momentum during the main sequence evolution; no signs of additional magnetic braking were found. The inclination angles of the rotational axes are randomly distributed, although an apparent excess of fast rotators with comparable inclination angles has been observed. We have found a rotation rate of v/v_crit_&gt;=0.5 for several stars, whose characteristics cannot be explained by current models. For the first time, we have derived the relationship between mass and rotation rate of mCP stars, and provide an analysis that links mass and rotation with magnetic field strength. Our sample is unique and offers crucial input for forthcoming evolutionary models that include the effects of magnetic fields for upper main sequence stars.</description><source format="bibcode">2017MNRAS.468.2745N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/468/2745</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+AS/103/1">J/A+AS/103/1 : ubvy Photometry of magnetic CP stars (Adelman+ 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/111/41">J/A+AS/111/41 : Photometry of magnetic CP stars (North+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/114/253">J/A+AS/114/253 : uvby Photometry of Magnetic CP Stars (Adelman+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/122/249">J/A+AS/122/249 : uvby photometry of 4 CP stars (Adelman, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/125/65">J/A+AS/125/65 : uvby photometry of 4 CP stars (Adelman, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/136/111">J/A+AS/136/111 : uvby photometry of 4 CP stars (Adelman+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/136/379">J/A+AS/136/379 : uvby photometry of 4 CP stars (Adelman+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/146/13">J/A+AS/146/13 : uvby photometry of 4 CP stars (Adelman, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/357/548">J/A+A/357/548 : ubvy Photometry of magnetic CP stars (Adelman+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/401/357">J/A+A/401/357 : uvby photometry of 2 Am and 2 mCP stars (Adelman+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/317">J/A+A/429/317 : uvby photometry of 1 HgMn and 3 mCP stars (Adelman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/435/1099">J/A+A/435/1099 : ubvy photometry of 4 magnetic CP stars (Adelman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Ap/46.234">J/other/Ap/46.234 : magnetic CP stars spatial distribution (Kudryavtsev+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/AstBu/62.244">J/other/AstBu/62.244 : Magnetic field in CP stars (Glagolevskij, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/450/763">J/A+A/450/763 : Evolutionary state of magnetic CP stars (Kochukhov+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/581/A138">J/A+A/581/A138 : Photometric variability in magnetic CP stars (Bernhard+, 2015</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/104">J/AJ/152/104 : New photometrically variable magnetic CP stars</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/468/2745</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/468/2745</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/468/2745</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/468/2745</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Per</name><description>Period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>f_Per</name><description>Source of Period (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Vmag</name><description>Visual magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E(B-V)</name><description>? Interstellar reddening</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logTeff</name><description>? Mean effective temperature</description><unit>log(K)</unit><ucd>phys.temperature.effective;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logTeff</name><description>? Error on logTeff</description><unit>log(K)</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_logTeff</name><description>? Number of individual Teff values</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>logL</name><description>? Luminosity</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logL</name><description>? Error on logL</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>? Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Mass</name><description>? Error on Mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Veq</name><description>? Equatorial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.eq</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_Veq</name><description>? Error on Veq</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>v/vcrit</name><description>? 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