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<ri:Resource created="2024-02-23T06:50:23Z" 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>Radial velocities of 123 active stars</title><shortName>J/AJ/166/16</shortName><identifier>ivo://CDS.VizieR/J/AJ/166/16</identifier><altIdentifier>doi:10.26093/cds/vizier.51660016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pass E.K.</name></creator><creator><name>Winters J.G.</name></creator><creator><name>Charbonneau D.</name></creator><creator><name>Irwin J.M.</name></creator><creator><name>Medina A.A.</name></creator><date role="Updated">2025-04-22T20:11:19Z</date><date role="Created">2024-02-23T06:50:23Z</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>m-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>stellar-masses</subject><subject>radial-velocity</subject><description>We present results from the volume-complete spectroscopic survey of 0.1-0.3M{sun} M-dwarfs within 15pc. This work discusses the active sample without close binary companions, providing a comprehensive picture of these 123 stars with H{alpha} emission stronger than -1{AA}. Our analysis includes rotation periods (including 31 new measurements), H{alpha} equivalent widths, rotational broadening, inclinations, and radial velocities, determined using high-resolution, multiepoch spectroscopic data from the TRES and CHIRON spectrographs supplemented by photometry from TESS and MEarth. Using this volume-complete sample, we establish that the majority of active, low-mass M-dwarfs are very rapid rotators: specifically, 74%{+/-}4% have rotation periods shorter than 2 days, while 19%{+/-}4% have intermediate rotation periods of 2-20 days, and the remaining 8%{+/-}3% have periods longer than 20 days. Among the latter group, we identify a population of stars with very high H{alpha} emission, which we suggest is indicative of dramatic spindown as these stars transition from the rapidly rotating mode to the slowly rotating one. We are unable to determine rotation periods for six stars and suggest that some of the stars without measured rotation periods may be viewed pole- on, as such stars are absent from the distribution of inclinations we measure; this lack notwithstanding, we recover the expected isotropic distribution of spin axes. Our spectroscopic and photometric data sets also allow us to investigate activity-induced radial-velocity variability, which we show can be estimated as the product of rotational broadening and the photometric amplitude of spot modulation.</description><source format="bibcode">2023AJ....166...16P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/166/16</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/IV/38">IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/390/567">J/MNRAS/390/567 : Magnetic field and velocity of mid M dwarfs (Morin+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1118">J/ApJ/720/1118 : i-band photometry of HAT-P-16 (Buchhave+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/407/2269">J/MNRAS/407/2269 : Polarisation of a sample of late M dwarfs (Morin+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/166">J/AJ/141/166 : HATNet variability survey of K and M dwarfs (Hartman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/728/48">J/ApJ/728/48 : Multicolor eclipse data for 6 new binaries (Kraus+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/48">J/ApJ/743/48 : Stars rotation periods &amp; Xray luminosities (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. 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