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<ri:Resource created="2019-03-25T14:18:29Z" 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 of 7 new member stars in Tucana II</title><shortName>J/ApJ/857/74</shortName><identifier>ivo://CDS.VizieR/J/ApJ/857/74</identifier><altIdentifier>doi:10.26093/cds/vizier.18570074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chiti A.</name></creator><creator><name>Frebel A.</name></creator><creator><name>Ji A.P.</name></creator><creator><name>Jerjen H.</name></creator><creator><name>Kim D.</name></creator><creator><name>Norris J.E.</name></creator><date role="Updated">2019-04-08T12:56:22Z</date><date role="Created">2019-03-25T14:18:29Z</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>chemical-abundances</subject><subject>radial-velocity</subject><subject>line-intensities</subject><description>We present chemical abundance measurements for seven stars with metallicities ranging from [Fe/H]=-3.3 to [Fe/H]=-2.4 in the TucanaII ultra-faint dwarf galaxy (UFD), based on high-resolution spectra obtained with the MIKE spectrograph on the 6.5m Magellan-Clay Telescope. For three stars, we present detailed chemical abundances for the first time. Of those, two stars are newly discovered members of Tucana II and were selected as probable members from deep narrowband photometry of the Tucana II UFD taken with the SkyMapper telescope. This result demonstrates the potential for photometrically identifying members of dwarf galaxy systems based on chemical composition. One new star was selected from the membership catalog of Walker+ (2016, J/ApJ/819/53). The other four stars in our sample have been reanalyzed, following additional observations. Overall, six stars have chemical abundances that are characteristic of the UFD stellar population. The seventh star shows chemical abundances that are discrepant from the other Tucana II members and an atypical, higher strontium abundance than what is expected for typical UFD stars. While unlikely, its strontium abundance raises the possibility that it may be a foreground metal-poor halo star with the same systemic velocity as Tucana II. If we were to exclude this star, Tucana II would satisfy the criteria to be a surviving first galaxy. Otherwise, this star implies that Tucana II has likely experienced somewhat extended chemical evolution.</description><source format="bibcode">2018ApJ...857...74C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/857/74</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/ApJ/645/613">J/ApJ/645/613 : Abundances of HD 221170 (Ivans+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/162/227">J/ApJS/162/227 : Transition probabilities for SmII (Lawler+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/51">J/ApJS/182/51 : Transitions of rare earth elements (Lawler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/80">J/ApJS/182/80 : Rare earth abundances (Sneden+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/331/474">J/AN/331/474 : Abundances of metal-poor stars (Frebel, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/560">J/ApJ/708/560 : Spectroscopy of UMa II and Coma Ber (Frebel+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/724/341">J/ApJ/724/341 : Nucleosynthesis of massive metal-free stars (Heger+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/350">J/ApJ/711/350 : Metal-poor giant Boo-1137 abundances (Norris+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/175">J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/124/140">J/PASP/124/140 : UBVRI Hp BT and VT photonic responses (Bessell+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/57">J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/61">J/ApJ/763/61 : Abundances of 7 red giants of BootesI (Gilmore+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/102">J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/767/134">J/ApJ/767/134 : Abundances of red giants in UFD galaxies (Vargas+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/786/74">J/ApJ/786/74 : EW measurements of 6 Segue 1 red giants (Frebel+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A146">J/A+A/562/A146 : Chemical abundances of 8 metal-poor stars (Ishigaki+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/571/A47">J/A+A/571/A47 : Linelist of CH in stellar atmospheres (Masseron+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/21">J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/2665">J/MNRAS/440/2665 : SDSS J021933.13+200830.2 spectroscopy (Roederer+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/147/136">J/AJ/147/136 : Stars of very low metal abundance. 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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>Name</name><description>Tucana II star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>Sp</name><description>Atomic species of absorption feature</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>f_Sp</name><description>Species corrected (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Nl</name><description>[1/99] Number of lines fit</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>loge</name><description>[0.5/8.5] Log number abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_[X/H]</name><description>Limit flag on [X/H]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[X/H]</name><description>[-4.9/-1.6] Log abundance relative to hydrogen</description><ucd>phys.abund;arith.zp</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>u_[X/H]</name><description>Uncertainty flag on [X/H]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_[X/Fe]</name><description>Limit flag on [X/Fe]</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>[X/Fe]</name><description>[-2.0/1.3] Log abundance relative to iron</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>u_[X/Fe]</name><description>Uncertainty flag on [X/Fe]; see text</description><ucd>meta.code.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>sigma</name><description>[0.1/0.7]? 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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>Name</name><description>Tucana II star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>lambda</name><description>[3783.5/6678] Rest wavelength of absorption feature</description><unit>0.1nm</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Sp</name><description>Atomic species of absorption feature</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>chi</name><description>[0/4.4]? 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