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<ri:Resource created="2002-02-17T13:20:30Z" 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 velocities of A-type stars. I.</title><shortName>J/A+A/381/105</shortName><identifier>ivo://CDS.VizieR/J/A+A/381/105</identifier><altIdentifier>doi:10.26093/cds/vizier.33810105</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Royer F.</name></creator><creator><name>Gerbaldi M.</name></creator><creator><name>Faraggiana R.</name></creator><creator><name>Gomez A.E.</name></creator><date role="Updated">2018-01-10T11:47:42Z</date><date role="Created">2002-02-17T13:20:30Z</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>early-type-stars</subject><subject>a-stars</subject><subject>galaxy-kinematics</subject><description>Within the scope of a Key Programme determining fundamental parameters of stars observed by HIPPARCOS, spectra of 525 B8 to F2-type stars brighter than V=8 have been collected at ESO. Fourier transforms of several line profiles in the range 4200-4500{AA} are used to derive vsini from the frequency of the first zero. Statistical analysis of the sample indicates that measurement error is a function of vsini and this relative error of the rotational velocity is found to be about 6% on average. The results obtained are compared with data from the literature. There is a systematic shift from standard values from Slk_7_5, which are 10 to 12% lower than our findings. Comparisons with other independent vsini values tend to prove that those from Slettebak et al. (1975ApJS...29..137S) are underestimated. This effect is attributed to the presence of binaries in the standard sample of Slettebak et al. (1975ApJS...29..137S), and to the model atmosphere they used.</description><source format="bibcode">2002A&amp;A...381..105R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/381/105</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/III/226">III/226 : Rotational Velocities of Stars (Glebocki+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/335/183">J/A+A/335/183 : Pleiades low-mass stars rotational velocities (Queloz+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/21">J/A+AS/126/21 : Velocities and duplicity of F-type dwarfs (Nordstroem+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/433">J/A+AS/139/433 : RV and vsini of evolved stars (de Medeiros+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/284/265">J/MNRAS/284/265 : Rotational Velocities of 373 OB stars (Howarth+ 1997)</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/A+A/381/105</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/381/105</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/381/105</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HD</name><description>HD number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>HIP</name><description>? HIP number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SpType</name><description>MK Spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>vsini</name><description>vsini</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>u_vsini</name><description>Uncertainty flag on vsini</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>sigma</name><description>? 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