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<ri:Resource created="2021-07-06T07:34:22Z" 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 Solar Neighborhood. XLVII. Mdwarfs with STIS</title><shortName>J/AJ/161/172</shortName><identifier>ivo://CDS.VizieR/J/AJ/161/172</identifier><altIdentifier>doi:10.26093/cds/vizier.51610172</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dieterich S.B.</name></creator><creator><name>Simler A.</name></creator><creator><name>Henry T.J.</name></creator><creator><name>Jao W.-C.</name></creator><date role="Updated">2024-10-11T20:10:04Z</date><date role="Created">2021-07-06T07:34:22Z</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>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>We use HST/STIS optical spectroscopy of 10 M-dwarfs in five closely separated binary systems to test models of M-dwarf structure and evolution. Individual dynamical masses ranging from 0.083 to 0.405M{sun} for all stars are known from previous work. We first derive temperature, radius, luminosity, surface gravity, and metallicity by fitting the BT-Settl atmospheric models. We verify that our methodology agrees with empirical results from long-baseline optical interferometry for stars of similar spectral types. We then test whether or not evolutionary models can predict those quantities given the stars' known dynamical masses and the conditions of coevality and equal metallicity within each binary system. We apply this test to five different evolutionary model sets: the Dartmouth models, the MESA/MIST models, the models of Baraffe et al., the PARSEC models, and the YaPSI models. We find marginal agreement between evolutionary model predictions and observations, with few cases where the models respect the condition of coevality in a self-consistent manner. We discuss the pros and cons of each family of models and compare their predictive power.</description><source format="bibcode">2021AJ....161..172D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/161/172</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/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/773">J/AJ/106/773 : Mass-luminosity relation (Henry+, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/327/1039">J/A+A/327/1039 : Structure and evolution of low-mass stars (Chabrier+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/413">J/AJ/129/413 : New high proper motion stars (-90&lt;DE47) (Subasavage+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/1658">J/AJ/130/1658 : High proper motion stars (-47&lt;{delta}&lt;00) (Subasavage+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/2898">J/AJ/133/2898 : New proper-motion stars (-90&lt;DE&lt; -47) (Finch+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/252">J/AJ/134/252 : New nearby white dwarf systems (Subasavage+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/A+ARV/18.67">J/other/A+ARV/18.67 : Accurate masses and radii of normal stars (Torres+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/21">J/AJ/141/21 : CCD distance estimates of SCR targets (Winters+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/10">J/AJ/142/10 : New proper motion stars 0.40"/yr&gt;pm&gt;=0.18"/yr (Boyd+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/92">J/AJ/142/92 : New proper motion stars with pm&gt;=0.18"/yr (Boyd+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/112">J/ApJ/757/112 : Stellar diameters. 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