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<ri:Resource created="2024-01-26T08:45:37Z" 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>Abundances in 16 red-giant in NGC 7789</title><shortName>J/AJ/165/245</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/245</identifier><altIdentifier>doi:10.26093/cds/vizier.51650245</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nagarajan N.</name></creator><creator><name>Sneden C.</name></creator><creator><name>Afsar M.</name></creator><creator><name>Pilachowski C.A.</name></creator><date role="Updated">2024-11-22T20:08:37Z</date><date role="Created">2024-01-26T08:45:37Z</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>giant-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>chemical-abundances</subject><description>We have gathered optical-region spectra, derived model atmosphere parameters, and computed elemental abundances for 15 red giant stars in the open cluster NGC7789. We focus on the light element group CNOLi that provides clues to evolutionary changes associated with internal fusion events and chemical mixing. We confirm and extend an early report that NGC7789 stars 193 and 301 have anomalously large Li abundances, and that these values are apparently unconnected to any other elements' abundances in these stars. A companion study of HeI{lambda}10830 lines in both field stars and cluster members shows that star 301 has a strong He feature while star 193 does not. Possible explanations for the large Li abundances of these stars include helium flash-induced mixing events and binary interactions at some past or present times. In either case an internal eruption of energy could cause fresh synthesis of lithium via the Cameron-Fowler Berillyum transport mechanism. Rapid transport of lithium to the outer layers may have created significant chromospheric transient disturbances, producing enough helium ionization to allow for the strong {lambda}10830 absorption in star 301.</description><source format="bibcode">2023AJ....165..245N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/245</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/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/110/1318">J/PASP/110/1318 : NGC 7789 CCD VI photometry (Gim+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/321/277">J/AN/321/277 : Effective temperatures of K-M giants (Strassmeier+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/431/933">J/A+A/431/933 : Abundances of NGC 7789 evolved stars (Tautvaisiene+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/328/938">J/AN/328/938 : Teff/line-depth ratio for ELODIE spectra (Biazzo+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A48">J/A+A/523/A48 : Gaia photometry (Jordi+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/A56">J/A+A/511/A56 : Abundances of five open clusters (Pancino+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/59">J/AJ/142/59 : Chemical abundance in 10 open clusters (Jacobson+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/446/3562">J/MNRAS/446/3562 : Abundances of red giants in NGC752 (Bocek Topcu+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/15">J/AJ/149/15 : Spectroscopy of NGC 7789 (Overbeek+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/580">J/MNRAS/463/580 : Abundances of red giants in NGC6940 (Bocek+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/618/A93">J/A+A/618/A93 : Gaia DR2 open clusters in Milky Way (Cantat-Gaudin+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/2000">J/MNRAS/484/2000 : Study of Lithium-rich giants with GALAH (Deepak+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/879/105">J/ApJ/879/105 : Effective temp of low-mass stars (Lopez-Valdivia+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/655/A23">J/A+A/655/A23 : Open cluster red clump stars Lit abundances (Magrini+, 2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/165/245</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/165/245</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/165/245</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/165/245</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/165/245</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Star 501 equivalent width</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW-637</name><description>[28/236]? Star 637 equivalent width</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW-669</name><description>[26/285]? Star 699 equivalent width</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW-765</name><description>[26/243]? Star 765 equivalent width</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW-970</name><description>[24/272]? 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