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<ri:Resource created="2018-11-20T13:23:26Z" 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>WOCS.LXXVI.Velocity &amp; abundances in NGC2506</title><shortName>J/AJ/155/138</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/138</identifier><altIdentifier>doi:10.26093/cds/vizier.51550138</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Anthony-Twarog B.J.</name></creator><creator><name>Lee-Brown D.B.</name></creator><creator><name>Deliyannis C.P.</name></creator><creator><name>Twarog B.A.</name></creator><date role="Updated">2019-01-07T08:47:50Z</date><date role="Created">2018-11-20T13:23:26Z</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>multiple-stars</subject><subject>giant-stars</subject><subject>radial-velocity</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><subject>line-intensities</subject><description>HYDRA spectra of 287 stars in the field of NGC 2506 from the turnoff through the giant branch are analyzed. With previous data, 22 are identified as probable binaries; 90 more are classified as potential non-members. Spectroscopic analyses of ~60 red giants and slowly rotating turnoff stars using line equivalent widths and a neural network approach lead to [Fe/H]=-0.27+/-0.07 (s.d.) and [Fe/H]=-0.27+/-0.06 (s.d.), respectively. Li abundances are derived for 145 probable single-star members, 44 being upper limits. Among turnoff stars outside the Li-dip, A(Li)=3.04+/-0.16 (s.d.), with no trend with color, luminosity, or rotation speed. Evolving from the turnoff across the subgiant branch, there is a well-delineated decline to A(Li)~1.25 at the giant branch base, coupled with the rotational spindown from between ~20 and 70 km/s to less than 20 km/s for stars entering the subgiant branch and beyond. A(Li) remains effectively constant from the giant branch base to the red giant clump level. A new member above the clump redefines the path of the first-ascent red giant branch; its Li is 0.6 dex below the first-ascent red giants. With one exception, all post-He-flash stars have upper limits to A(Li), at or below the level of the brightest first-ascent red giant. The patterns are in excellent qualitative agreement with the model predictions for low/intermediate-mass stars which undergo rotation-induced mixing at the turnoff and subgiant branch, first dredge-up, and thermohaline mixing beyond the red giant bump.</description><source format="bibcode">2018AJ....155..138A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/138</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/J/A+AS/113/299">J/A+AS/113/299 : Abundances and velocities for cluster giants (Minniti 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/1486">J/AJ/122/1486 : NGC 2451A proper motions and membership (Platais+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/382/899">J/A+A/382/899 : BVI photometry in M67 (Stassun+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/601">J/AJ/124/601 : Absolute positions and proper motions in NGC 188</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2922">J/AJ/126/2922 : Astrometry and membership in NGC 188 (Platais+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/461/509">J/A+A/461/509 : Membership and spectroscopy of IC 2391 (Platais+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/484/609">J/A+A/484/609 : BVI photometry and proper motions in M67 (Yadav+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/2264">J/AJ/135/2264 : Stellar radial velocities in NGC 188 (Geller+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/391/1482">J/MNRAS/391/1482 : BVIc photometry of Trumpler 20 (Platais+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3743">J/AJ/137/3743 : Spectroscopic binary orbits in NGC 188 (Geller+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/5086">J/AJ/137/5086 : NGC 188 V12 VI light curves (Meibom+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/138/159">J/AJ/138/159 : NGC 6819 stellar radial-velocity and photometry</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/695/679">J/ApJ/695/679 : Stellar rotation in M35 (Meibom+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/515/A100">J/A+A/515/A100 : VI light curves of NGC 1039 solar-type stars (James+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/1383">J/AJ/139/1383 : Radial velocities in M35 (NGC 2168) (Geller+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/139/2034">J/AJ/139/2034 : NGC 6253 stars equivalent widths (Anthony-Twarog+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/115">J/ApJ/733/115 : Rotation periods and membership in M34 (Meibom+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/1024">J/MNRAS/413/1024 : Deep proper-motion survey of Blanco 1 (Platais+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/419/1350">J/MNRAS/419/1350 : Red giants abundances in 4 open clusters (Reddy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/43">J/AJ/146/43 : WIYN open cluster study. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>WEBDA</name><description>[1106/7135] WEBDA identification number (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RAJ2000</name><description>Right Ascension in decimal degrees (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination in decimal degrees (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Prob</name><description>[0/0.95]? Membership probability (Chiu &amp; Van Altena 1981ApJ...243..827C)</description><ucd>stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HRV</name><description>[-45.9/136] Heliocentric radial velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_HRV</name><description>[0.1/19.7] Uncertainty in HRV</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vsini</name><description>[7/110.2] Rotational velocity</description><unit>km/s</unit><ucd>phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_vsini</name><description>[0.1/10.9] Uncertainty in vsini</description><unit>km/s</unit><ucd>stat.error;phys.veloc.rotat</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B-V</name><description>[0.196/1.756] B-V color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vmag</name><description>[11.252/15.584] V band magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Class</name><description>Membership classification (2)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column></table><table><name>J/AJ/155/138/table3</name><description>Abundances for NGC 2506 stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>WEBDA</name><description>[1108/7128] WEBDA identification number (G1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff-NN</name><description>[4546/5768]? Effective temperature derived with ANNA code</description><unit>K</unit><ucd>meta.code;phys.temperature</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>[Fe/H]-NN</name><description>[-0.48/0.34]? Metallicity derived with ANNA code</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]-RS</name><description>[-0.55/0.24] Median metallicity derived with ROBOSPECT code</description><unit>log(Sun)</unit><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MAD</name><description>[0.01/0.29] Median absolute deviation for Fe abundance</description><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>NFe</name><description>[5/17] Number of Fe lines measured</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Ca/H]</name><description>[-0.54/0.28]? Ca abundance derived with ROBOSPECT code</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Si/H]</name><description>[-1.14/0.28] Si abundance derived with ROBOSPECT code</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ni/H]</name><description>[-0.85/0.31] Ni abundance derived with ROBOSPECT code</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Ni/H]</name><description>[0.01/0.19] Uncertainty in [Ni/H]</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff-ph</name><description>[4504/7079] Photometric effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[1.9/3.7] Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>xi</name><description>[1.31/2.3] Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/155/138/table4</name><description>Lithium abundances for NGC 2506 stars</description><column><name>l_A(Li)</name><description>[&lt;] Limit flag on A(Li)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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