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<ri:Resource created="2015-12-10T13:30:10Z" 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>IN-SYNC. III. Radial velocities of IC348 stars</title><shortName>J/ApJ/807/27</shortName><identifier>ivo://CDS.VizieR/J/ApJ/807/27</identifier><altIdentifier>doi:10.26093/cds/vizier.18070027</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cottaar M.</name></creator><creator><name>Covey K.R.</name></creator><creator><name>Foster J.B.</name></creator><creator><name>Meyer M.R.</name></creator><creator><name>Tan J.C.</name></creator><creator><name>Nidever D.L.,Drew Chojnowski S.</name></creator><creator><name>da Rio N.</name></creator><creator><name>Flaherty K.M.</name></creator><creator><name>Frinchaboy P.M.</name></creator><creator><name>Majewski S.,Skrutskie M.F.</name></creator><creator><name>Wilson J.C.</name></creator><creator><name>Zasowski G.</name></creator><date role="Updated">2017-09-20T05:13:46Z</date><date role="Created">2015-12-10T13:30:10Z</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>radial-velocity</subject><description>Most field stars will have encountered the highest stellar density and hence the largest number of interactions in their birth environment. Yet the stellar dynamics during this crucial phase are poorly understood. Here we analyze the radial velocities measured for 152 out of 380 observed stars in the 2-6Myr old star cluster IC 348 as part of the SDSS-III APOGEE. The radial velocity distribution of these stars is fitted with one or two Gaussians, convolved with the measurement uncertainties including binary orbital motions. Including a second Gaussian improves the fit; the high-velocity outliers that are best fit by this second component may either (1) be contaminants from the nearby Perseus OB2 association, (2) be a halo of ejected or dispersing stars from IC 348, or (3) reflect that IC 348 has not relaxed to a Gaussian velocity distribution. We measure a velocity dispersion for IC 348 of 0.72+/-0.07km/s (or 0.64+/-0.08km/s if two Gaussians are fitted), which implies a supervirial state, unless the gas contributes more to the gravitational potential than expected. No evidence is found for a dependence of this velocity dispersion on distance from the cluster center or stellar mass. We also find that stars with lower extinction (in the front of the cloud) tend to be redshifted compared with stars with somewhat higher extinction (toward the back of the cloud). This data suggest that the stars in IC 348 are converging along the line of sight. We show that this correlation between radial velocity and extinction is unlikely to be spuriously caused by the small cluster rotation of 0.024+/-0.013km/s/arcmin or by correlations between the radial velocities of neighboring stars. This signature, if confirmed, will be the first detection of line of sight convergence in a star cluster. Possible scenarios for reconciling this convergence with IC 348's observed supervirial state include: (a) the cluster is fluctuating around a new virial equilibrium after a recent disruption due to gas expulsion or a merger event, or (b) the population we identify as IC 348 results from the chance alignment of two sub-clusters converging along the line of sight. Additional measurements of tangential and radial velocities in IC 348 will be important for clarifying the dynamics of this region and informing models of the formation and evolution of star clusters.</description><source format="bibcode">2015ApJ...807...27C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/807/27</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/197">II/197 : ISM towards IC 348 and Per OB2 (Cernis, 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/136">J/ApJ/799/136 : IN-SYNC. II. 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SFR (Bell+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/66">J/AJ/145/66 : Spitzer light curves of YSOs in IC 348 (Flaherty+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/554/A55">J/A+A/554/A55 : C^18^O(1-0) and N_2_H^+^(1-0) in L1495/B213 (Hacar+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/539/A64">J/A+A/539/A64 : X-ray data for IC 348 young stars (Alexander+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A135">J/A+A/537/A135 : X-ray view of IC348 (Stelzer+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/44">J/ApJ/754/44 : The AstraLux Large M-dwarf Survey (Janson+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/1">J/ApJS/190/1 : A survey of stellar families (Raghavan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/181/321">J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/703">J/AJ/138/703 : Deep MIPS observations of IC 348 nebula (Currie+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/411">J/AJ/134/411 : Properties of IC 348 members (Muench+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1574">J/AJ/131/1574 : Infrared photometry of IC348 members (Lada+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/649/862">J/ApJ/649/862 : IR phot. of IC 348 pre-main-sequence stars (Cieza+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/597/555">J/ApJ/597/555 : IR photometry of IC 348 young brown dwarfs (Mainzer+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/409/147">J/A+A/409/147 : J magnitude of IC 348 brown dwarfs (Preibisch+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/593/1093">J/ApJ/593/1093 : IC 348 membership (Luhman+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/866">J/AJ/122/866 : X-ray sources in IC 348 from Chandra (Preibisch+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/541/977">J/ApJ/541/977 : HST observations of low-mass stars in IC 348 (Najita+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/525/466">J/ApJ/525/466 : Young low-mass stars &amp; 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