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<ri:Resource created="2019-09-30T15:38:01Z" 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>GOBELINS. V. Kinematics of Perseus</title><shortName>J/ApJ/865/73</shortName><identifier>ivo://CDS.VizieR/J/ApJ/865/73</identifier><altIdentifier>doi:10.26093/cds/vizier.18650073</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ortiz-Leon G.N.</name></creator><creator><name>Loinard L.</name></creator><creator><name>Dzib S.A.</name></creator><creator><name>Galli P.A.B.</name></creator><creator><name>Kounkel M.,Mioduszewski A.J.</name></creator><creator><name>Rodriguez L.F.</name></creator><creator><name>Torres R.M.</name></creator><creator><name>Hartmann L.</name></creator><creator><name>Boden A.F.,Evans N.J.</name></creator><creator><name>Briceno C.</name></creator><creator><name>Tobin J.J.</name></creator><date role="Updated">2020-03-26T14:18:40Z</date><date role="Created">2019-09-30T15:38:01Z</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>proper-motions</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>radial-velocity</subject><subject>infrared-sources</subject><subject>open-star-clusters</subject><subject>star-forming-regions</subject><description>We derive the distance and structure of the Perseus molecular cloud by combining trigonometric parallaxes from Very Long Baseline Array (VLBA) observations, taken as part of the GOBELINS survey and Gaia Data Release 2. Based on our VLBA astrometry, we obtain a distance of 321+/-10pc for IC 348. This is fully consistent with the mean distance of 320+/-26 measured by Gaia. The VLBA observations toward NGC 1333 are insufficient to claim a successful distance measurement to this cluster. Gaia parallaxes, on the other hand, yield a mean distance of 293+/-22pc. Hence, the distance along the line of sight between the eastern and western edges of the cloud is ~30pc, which is significantly smaller than previously inferred. We use Gaia proper motions and published radial velocities to derive the spatial velocities of a selected sample of stars. The average velocity vectors with respect to the LSR are (u,v,w)=(-6.1+/-1.6, 6.8+/-1.1, -0.9+/-1.2) and (-6.4+/-1.0, 2.1+/-1.4, -2.4+/-1.0)km/s for IC 348 and NGC 1333, respectively. Finally, our analysis of the kinematics of the stars has shown that there is no clear evidence of expansion, contraction, or rotational motions within the clusters.</description><source format="bibcode">2018ApJ...865...73O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/865/73</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/I/347">I/347 : 1.33 billion stars distances in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/117/354">J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/2496">J/AJ/135/2496 : Near-IR survey of Class I protostars (Connelley+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/674/336">J/ApJ/674/336 : Spitzer observations of NGC 1333 (Gutermuth+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/692/973">J/ApJ/692/973 : Protostars in Perseus, Serpens and Ophiuchus (Enoch+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/710/1247">J/ApJ/710/1247 : Dense cores in Gould Belt clouds (Sadavoy+, 2010)</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/ApJ/794/125">J/ApJ/794/125 : IN-SYNC. 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Perseus region (Pech+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/73">J/ApJ/818/73 : Protostars in the Perseus molecular cloud (Tobin+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/142">J/ApJ/834/142 : Gould's Belt Distances Survey. II. OMC (Kounkel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/859/33">J/ApJ/859/33 : GOBELINS. IV. VLBA obs. of Taurus (Galli+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/84">J/AJ/156/84 : APOGEE-2 survey of Orion Complex. II. 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