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<ri:Resource created="2023-02-10T13:06:20Z" 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>Galactic disc enrichment with Mo and Ru</title><shortName>J/MNRAS/489/1697</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/489/1697</identifier><altIdentifier>doi:10.26093/cds/vizier.74891697</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mishenina T.</name></creator><creator><name>Pignatari M.</name></creator><creator><name>Gorbaneva T.</name></creator><creator><name>Travaglio C.</name></creator><creator><name>Cote B.,Thielemann F.-K.</name></creator><creator><name>Soubiran C.</name></creator><date role="Updated">2024-08-20T20:12:38Z</date><date role="Created">2023-02-10T13:06:20Z</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>metallicity</subject><subject>chemical-abundances</subject><subject>effective-temperature</subject><subject>late-type-stars</subject><subject>milky-way-galaxy</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We present new observational data for the heavy elements molybdenum (Mo, Z=42) and ruthenium (Ru, Z=44) in F-, G-, and K-stars belonging to different substructures of the Milky Way. The range of metallicity covered is -1.0&lt;[Fe/H]&lt;+0.3. The spectra of Galactic disc stars have a high resolution of 42000 and 75000 and signal-to-noise ratio better than 100. Mo and Ru abundances were derived by comparing the observed and synthetic spectra in the region of Mo I lines at 5506, 5533{AA} for 209 stars and Ru I lines at 4080, 4584, 4757{AA} for 162 stars using the LTE approach. For all the stars, the Mo and Ru abundance determinations are obtained for the first time with an average error of 0.14dex. This is the first extended sample of stellar observations for Mo and Ru in the Milky Way disc, and together with earlier observations in halo stars it is pivotal in providing a complete picture of the evolution of Mo and Ru across cosmic time-scales.</description><source format="bibcode">2019MNRAS.489.1697M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/489/1697</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></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/489/1697/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.6532667</ra><dec>29.0215036</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/49 60 100 137 237 309 377 455 684 742 819 918 987 1028 1084 1247 1330 1341 1530 1728 1827 1875 2167 2169 2317 2366 2472 2476 2491 2622 2652 2697 2923 3020 3102 3258 3313 3372 3509 3639 3662 3683 3691 3780 3786 3809 3979 4079 4241 4278 4591 4735 4762 4942 5009 5304 5309 5413 5498 5522 5726 5824 5932 6025 6217 6226 6273 6287 6385 6398 6409 6523 6662 6766 6926 6953 7354 7443 7763 8094 8224 8357 8466 8663 8995 9072 9476 9492 9662 9679 9801 9843 9873 10004 10062 10325 10375 10518 10812 10899 10914 11126 11142 11150 11165 11633 11713 11806 11834 12228 12282 12388 12494 12592 12654 12704 12856 12890 12944 12983 13036 13075 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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>[Mo/Fe]</name><description>? Molybdenum to Fe abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Mo/Fe]</name><description>? Error on [Mo/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>More</name><description>Parameters comparison with litterature</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>Star name (HD or BD)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>primary</flag></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>Iron to hydrogen abundance ratio</description><ucd>phys.abund.Fe;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vt</name><description>Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ru/Fe]</name><description>? Ruthenium to Fe abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[Ru/Fe]</name><description>? 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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>HD star name (NNNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Teffo</name><description>Effective temperature determined in this paper</description><unit>K</unit><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>loggo</name><description>Surface gravity determined in this paper</description><unit>log(cm.s**-2)</unit><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]o</name><description>Fe to H abundance ratio determined in this paper</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teffl</name><description>Effective temperature from litterature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggl</name><description>Surface gravity from litterature</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]l</name><description>Fe to H abundance ratio from litterature</description><ucd>phys.abund.Fe;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DTeff</name><description>Difference between Teffo and Teffl (Teffo-Teffl)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dlogg</name><description>Difference between loggo and loggl (loggo-loggl)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>D[Fe/H]</name><description>Difference between [Fe/H]o and [Fe/H]l ([Fe/H]o-[Fe/H]l)</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ref</name><description>References for Teffl, loggl and [Fe/H]l</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="68*">char</dataType></column></table></schema></tableset></ri:Resource>