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<ri:Resource created="2018-09-26T12:29:27Z" 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>The rotation of M dwarfs observed by APOGEE</title><shortName>J/AJ/155/38</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/38</identifier><altIdentifier>doi:10.26093/cds/vizier.51550038</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gilhool S.H.</name></creator><creator><name>Blake C.H.</name></creator><creator><name>Terrien R.C.</name></creator><creator><name>Bender C.</name></creator><creator><name>Mahadevan S.,Deshpande R.</name></creator><date role="Updated">2019-01-07T09:21:15Z</date><date role="Created">2018-09-26T12:29:27Z</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>dwarf-stars</subject><subject>m-stars</subject><subject>late-type-stars</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><description>We present the results of a spectroscopic analysis of rotational velocities in 714 M-dwarf stars observed by the SDSS-III Apache Point Galactic Evolution Experiment (APOGEE) survey. We use a template-fitting technique to estimate v sin i while simultaneously estimating log g, [M/H], and T_eff_. We conservatively estimate that our detection limit is 8 km/s. We compare our results to M-dwarf rotation studies in the literature based on both spectroscopic and photometric measurements. Like other authors, we find an increase in the fraction of rapid rotators with decreasing stellar temperature, exemplified by a sharp increase in rotation near the M4 transition to fully convective stellar interiors, which is consistent with the hypothesis that fully convective stars are unable to shed angular momentum as efficiently as those with radiative cores. We compare a sample of targets observed both by APOGEE and the MEarth transiting planet survey and find no cases where the measured v sin i and rotation period are physically inconsistent, requiring sin i&gt;1. We compare our spectroscopic results to the fraction of rotators inferred from photometric surveys and find that while the results are broadly consistent, the photometric surveys exhibit a smaller fraction of rotators beyond the M4 transition by a factor of ~2. We discuss possible reasons for this discrepancy. Given our detection limit, our results are consistent with a bimodal distribution in rotation that is seen in photometric surveys.</description><source format="bibcode">2018AJ....155...38G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/38</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/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/581">J/A+A/331/581 : Rotation and activity in field M dwarfs (Delfosse+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/704/975">J/ApJ/704/975 : Rotational velocities for M dwarfs (Jenkins+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/407/1657">J/MNRAS/407/1657 : Rotation velocities of dwarf M stars (Houdebine, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/93">J/AJ/143/93 : Rotational velocities in early-M stars (Reiners+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/156">J/AJ/146/156 : APOGEE M-dwarf survey. I. First year velocities</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/432/1203">J/MNRAS/432/1203 : Rotation periods of M-dwarf stars (McQuillan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weights for the 15 APOGEE chemical elements</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/460/2611">J/MNRAS/460/2611 : APOGEE K and M dwarfs (Schmidt+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/1844">J/MNRAS/463/1844 : M dwarfs rotation-activity relation (Stelzer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/837/96">J/ApJ/837/96 : Rotation-Activity Correlations in K-M dwarfs II.</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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