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<ri:Resource created="2011-01-11T10:02:12Z" 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>Velocities of M67 main-sequence and giant stars</title><shortName>J/A+A/526/A127</shortName><identifier>ivo://CDS.VizieR/J/A+A/526/A127</identifier><altIdentifier>doi:10.26093/cds/vizier.35260127</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pasquini L.</name></creator><creator><name>Melo C.</name></creator><creator><name>Chavero C.</name></creator><creator><name>Dravins D.</name></creator><creator><name>Ludwig H.-G.</name></creator><creator><name>Bonifacio P.,De La Reza R.</name></creator><date role="Updated">2017-12-07T07:26:49Z</date><date role="Created">2011-01-11T10:02:12Z</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>dwarf-stars</subject><subject>giant-stars</subject><subject>radial-velocity</subject><description>Precise analyses of stellar radial velocities is able to reveal intrinsic causes of the wavelength shifts of spectral lines (other than Doppler shifts due to radial motion), such as gravitational redshifts and convective blueshifts. Aims. Gravitational redshifts in solar-type main-sequence stars are expected to be some 500m/s greater than those in giants. 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