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<ri:Resource created="2017-03-22T07:37:06Z" 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>Iron-peak elements in solar neighbourhood</title><shortName>J/A+A/600/A22</shortName><identifier>ivo://CDS.VizieR/J/A+A/600/A22</identifier><altIdentifier>doi:10.26093/cds/vizier.36000022</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mikolaitis S.</name></creator><creator><name>de Laverny P.</name></creator><creator><name>Recio-Blanco A.</name></creator><creator><name>Hill V.</name></creator><creator><name>Worley C.C.,de Pascale M.</name></creator><date role="Updated">2017-04-11T12:09:13Z</date><date role="Created">2017-03-22T07:37:06Z</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>spectroscopy</subject><subject>chemical-abundances</subject><description>The aim of this paper is to characterise the abundance patterns of five iron-peak elements (Mn, Fe, Ni, Cu, and Zn) for which the stellar origin and chemical evolution are still debated. We automatically derived iron peak (Mn, Fe, Ni, Cu, and Zn) and alpha element (Mg) chemical abundances for 4666 stars. We used the bimodal distribution of [Mg/Fe] to chemically classify sample stars into different Galactic substructures: thin disc, metal-poor and high-alpha metal rich, high-alpha and low-alpha metal-poor populations. High-alpha and low-alpha metal-poor populations are fully distinct in Mg, Cu, and Zn. Thin disc trends of [Ni/Fe] and [Cu/Fe] are very similar and show a small increase at supersolar metallicities. Thin and thick disc trends of Ni and Cu are very similar and indistinguishable. Mn looks different from Ni and Cu. [Mn/Fe] trends of thin and thick discs actually have noticeable differences: the thin disc is slightly Mn richer than the thick disc. [Zn/Fe] trends look very similar to those of [alpha/Fe] trends. The dispersion of results in both discs is low (~0.05dex for [Mg, Mn, and Cu/Fe]) and is even much lower for [Ni/Fe] (~0.035dex). Zn is an alpha-like element and could be used to separate thin and thick disc stars. [Mn/Mg] ratio could also be a very good tool for tagging Galactic substructures. Some models can partially reproduce the observed Mg, Zn, and, Cu behaviours. Models mostly fail to reproduce Mn and Ni in all metallicity domains, however, models adopting yields normalised from solar chemical properties reproduce Mn and Ni better, suggesting that there is still a lack of realistic theoretical yields of some iron-peak elements. Very low scatter (~0.05dex) in thin and thick disc sequences could provide an observational constrain for Galactic evolutionary models that study the efficiency of stellar radial migration.</description><source format="bibcode">2017A&amp;A...600A..22M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/600/A22</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+A/595/A18">J/A+A/595/A18 : Lithium abundances in AMBRE stars (Guiglion+, 2016)</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/A+A/600/A22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/600/A22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/600/A22</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/600/A22</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/600/A22</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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46685 46687 46702 46705 46709 46713 46722 46724 46728 46734 46768 46776-46777 46784 46788 46800 46803 46829-46830 46844 46856 46874 46881 46887 46921 46923 46925 46927 46936 46944 46967 46971 46978 46983 46994 46997 47004 47020 47022 47030 47037 47039 47045 47061 47065 47070 47073 47077 47092-47094 47107 47137 47157 47176 47181 47184 47198 47207 47211 47223 47253-47254 47308 47335 47339 47354 47364 47377 47387 47390 47398 47407 47409 47453 47510 47543 47550 47567 47575 47580 47584 47589-47590 47600 47629 47647 47655 47663 47674 47676 47706 47712 47715 47740 47780 47791 47795 47803 47809 47819 47832 47858 47894 47898 47903 47930 47935 47942 47977 47985 47994 48014 48022 48037 48050 48061 48065 48082 48105 48113 48133 48162 48172-48173 48177 48182-48183 48188 48205 48218 48238 48245-48246 48249 48260 48274 48282 48291 48310 48327 48345 48349-48350 48361-48362 48371 48388 48394 48402 48405 48421 48450 48469 48478 48481 48486 48490 48513-48514 48519 48530 48535 48545 48565 48572 48581 48583 48607 48652 48658 48664 48672 48679 48704-48705 48707 48727 48731 48736 48757 48768 48773 48792 48807 48821 48846 48865 48870-48871 48882 48893 48926 48943 48964 48980 48998 49001 49010 49036 49042 49060 49064 49078 49097 49108 49113-49114 49128</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/600/A22?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/600/A22/table5</name><description>Abundances of 4666 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>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Spect</name><description>Sepctrograph identification name, HARPS or FEROS</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>[MgI/Fe]</name><description>Abundance [MgI/Fe] (Z=12)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[MgI/Fe]</name><description>rms uncertainty of Mg1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[MnI/Fe]</name><description>? Abundance [MnI/Fe] (Z=25)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[MnI/Fe]</name><description>? rms uncertainty of Mn1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[FeI/H]</name><description>Abundance [Fe1/H] (Z=26)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeI/H]</name><description>rms uncertainty of Fe1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[FeII/H]</name><description>? Abundance [FeII/H] (Z=26)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[FeII/H]</name><description>? rms uncertainty of Fe2 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[NiI/Fe]</name><description>? Abundance [NiI/Fe] (Z=28)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[NiI/Fe]</name><description>? rms uncertainty of Ni1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[CuI/Fe]</name><description>? Abundance [CuI/Fe] (Z=29)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[CuI/Fe]</name><description>? rms uncertainty of Cu1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[ZnI/Fe]</name><description>? Abundance [ZnI/Fe] (Z=30)</description><unit>log(Sun)</unit><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[ZnI/Fe]</name><description>? rms uncertainty of Zn1 abundance</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GC</name><description>ID of the Galactic component (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column></table></schema></tableset></ri:Resource>