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<ri:Resource created="2023-09-28T15:29:00Z" status="active" updated="2025-06-13T15:25:00Z" 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>Lithium and beryllium in Gaia-Enceladus galaxy</title><shortName>J/MNRAS/496/2902</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/496/2902</identifier><altIdentifier>doi:10.26093/cds/vizier.74962902</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Molaro P.</name></creator><creator><name>Cescutti G.</name></creator><creator><name>Fu X.</name></creator><date role="Updated">2025-02-20T20:16:01Z</date><date role="Created">2023-09-28T15:29:00Z</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>halo-stars</subject><subject>dwarf-galaxies</subject><subject>metallicity</subject><subject>chemically-peculiar-stars</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><description>Data from Gaia DR2 and The Apache Point Observatory Galactic Evolution Experiment surveys revealed a relatively new component in the inner Galactic halo, which is likely the dynamical remnant of a disrupted dwarf galaxy named Gaia-Enceladus that collided with the Milky Way about 10Gyr ago. This merging event offers an extraordinary opportunity to study chemical abundances of elements in a dwarf galaxy, since they are generally hampered in external galaxies. Here, we focus on ^7^Li and ^9^Be in dwarf stars that are out of reach even in Local Group galaxies. Searching in GALAH, Gaia-ESO survey and in literature, we found several existing ^7^Li abundance determinations of stars belonging to the Gaia-Enceladus galaxy. The ^7^Li abundances of stars at the low metallicity end overlap with those of the Galactic halo. These are effective extragalactic ^7^Li measurements, which suggest that the ^7^Li Spite plateau is universal, as is the cosmological ^7^Li problem. We found a ^7^Li-rich giant out of 101 stars, which suggests a small percentage similar to that of the Milky Way. We also collect ^9^Be abundance for a subsample of 25 Gaia-Enceladus stars from literature. Their abundances share the Galactic [Be/H] values at the low metallicity end but grow slower with [Fe/H] and show a reduced dispersion. This suggests that the scatter observed in the Milky Way could reflect the different ^9^Be evolution patterns of different stellar components that are mixed-up in the Galactic halo.</description><source format="bibcode">2020MNRAS.496.2902M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/496/2902</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/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/478/4513">J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)</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/MNRAS/496/2902</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/496/2902</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/496/2902</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/496/2902</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/496/2902</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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41345 42252 42259 42649 42652 42735 43127 43249 43306 43309 43666 43916 44021 44045 44542 44922 45141 45147 45183 45330 45336 45340 45360 45411 45418 45470 45489 45500 45504 45549 45905 45976 46031 46053 46066 46096 46152 46625 46630 46651 46758 47111 47246 47459 47484 47501 47538 47568 47590 47734 47814 48245 48583 48736 48968</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/496/2902?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/496/2902/table1</name><description>Gaia-Enceladus candidate stars with Li and Be abundances measured from literature with log(g)&gt;3.65 and T_eff_&gt;5700K</description><column><name>More</name><description>Link to Table 2</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><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>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>GaiaDR2</name><description>Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd><flag>primary</flag></column><column><name>Name</name><description>Star name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Fe/H abundance ratio</description><ucd>phys.abund.Fe;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[O/H]</name><description>? O/H abundance ratio (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A(Li)</name><description>? Lithium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]Be</name><description>? Fe/H abundance ratio from the reference with Beryllium abundance measurements</description><ucd>phys.abund.Fe;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Fe/H]Be</name><description>? Error on [Fe/H]Be</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A(Be)</name><description>? Beryllium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A(Be)</name><description>? Error on A (Be)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>References (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/MNRAS/496/2902/table2</name><description>Kinematical properties of the selected Gaia-Enceladus candidates</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>GaiaDR2</name><description>Gaia DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>Name</name><description>Star name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Energy</name><description>Energy from Helmi et al. (2018Natur.563...85H)</description><unit>km**2.s**-2</unit><ucd>phys.energy</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Lz</name><description>Angular momentum in the Z direction from Helmi et al. 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