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<ri:Resource created="2024-06-28T07:43:19Z" 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>LMI and LDT observation of Berkeley 50 members</title><shortName>J/AJ/167/262</shortName><identifier>ivo://CDS.VizieR/J/AJ/167/262</identifier><altIdentifier>doi:10.26093/cds/vizier.51670262</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Speckert M.</name></creator><creator><name>Massey P.</name></creator><creator><name>Skiff B.A.</name></creator><date role="Updated">2024-11-06T20:20:15Z</date><date role="Created">2024-06-28T07:43:19Z</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>b-stars</subject><subject>supergiant-stars</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>trigonometric-parallax</subject><subject>proper-motions</subject><description>We observed the Galactic open cluster Berkeley-50 in order to determine its stellar content, distance, and age. We obtained UBV photometry of 1145 stars in a 12.3x12.3' field, and used Gaia proper motions and parallaxes to identify 64 members, of which we obtained spectra of the 17 brightest members. The majority of the observed population we classified as Bdwarfs, with the exception of a newly identified red supergiant star, which our spectroscopy shows has a B-type companion. Our study establishes the distance as 3.8kpc, with an average color-excess E(B-V)=0.9. Comparison of the physical properties of the cluster with the Geneva evolutionary tracks places the age of the cluster as 50-60Myr, with its most massive members being ~7M{sun}.</description><source format="bibcode">2024AJ....167..262S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/167/262</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/III/195">III/195 : Atlas of Optical Spectral Classification OB Stars (Walborn+ 1990)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/183">II/183 : UBVRI Photometric Standards (Landolt 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</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/ApJ/469/355">J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/113/1733">J/AJ/113/1733 : Orion Nebula Cluster population (Hillenbrand 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/576/880">J/ApJ/576/880 : CCD UBV photometry of h and {chi} Per (Slesnick+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/389/285">J/MNRAS/389/285 : Proper motions &amp; JHK of 24 Berkeley clusters (Tadross, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/537/A146">J/A+A/537/A146 : Stellar models with rot. 0.8&lt;M&lt;120, Z=0.014 (Ekstrom+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/543/A156">J/A+A/543/A156 : Milky Way global survey of star clusters (Kharchenko+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/121">J/AJ/156/121 : Catalog of 518 likely open cluster NGC6405 member (Gao, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/873/91">J/ApJ/873/91 : Interferometric obs. 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