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<ri:Resource created="2021-10-12T07:38:40Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>RAVE J183013.5-455510 equivalent-width measurements</title><shortName>J/ApJ/897/78</shortName><identifier>ivo://CDS.VizieR/J/ApJ/897/78</identifier><altIdentifier>doi:10.26093/cds/vizier.18970078</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Placco V.M.</name></creator><creator><name>Santucci R.M.</name></creator><creator><name>Yuan Z.</name></creator><creator><name>Mardini M.K.</name></creator><creator><name>Holmbeck E.M.</name></creator><creator><name>Wang X.,Surman R.</name></creator><creator><name>Hansen T.T.</name></creator><creator><name>Roederer I.U.</name></creator><creator><name>Beers T.C.</name></creator><creator><name>Choplin A.</name></creator><creator><name>Ji A.P.,Ezzeddine R.</name></creator><creator><name>Frebel A.</name></creator><creator><name>Sakari C.M.</name></creator><creator><name>Whitten D.D.</name></creator><creator><name>Zepeda J.</name></creator><date role="Updated">2022-03-15T04:12:46Z</date><date role="Created">2021-10-12T07:38:40Z</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>chemically-peculiar-stars</subject><subject>chemical-abundances</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We report on the spectroscopic analysis of RAVE-J183013.5-455510, an extremely metal-poor star, highly enhanced in CNO, and with discernible contributions from the rapid neutron-capture process. There is no evidence of binarity for this object. At [Fe/H]=-3.57, this star has one of the lowest metallicities currently observed, with 18 measured abundances of neutron-capture elements. The presence of Ba, La, and Ce abundances above the solar system r-process predictions suggests that there must have been a non-standard source of r-process elements operating at such low metallicities. One plausible explanation is that this enhancement originates from material ejected at unusually high velocities in a neutron star merger event. We also explore the possibility that the neutron-capture elements were produced during the evolution and explosion of a rotating massive star. In addition, based on comparisons with yields from zero-metallicity faint supernova, we speculate that RAVE-J1830-4555 was formed from a gas cloud pre-enriched by both progenitor types. From analysis based on Gaia DR2 measurements, we show that this star has orbital properties similar to the Galactic metal-weak thick-disk stellar population.</description><source format="bibcode">2020ApJ...897...78P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/897/78</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/III/279">III/279 : RAVE 5th data release (Kunder+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/349">I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/652/1585">J/ApJ/652/1585 : Bright metal-poor stars from HES survey (Frebel+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/492">J/ApJ/655/492 : Equivalent widths of 26 metal-poor stars (Aoki+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2050">J/AJ/136/2050 : SEGUE stellar parameter pipeline. 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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>Ion</name><description>Species</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>lambda</name><description>[3360/8335] Wavelength, Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ExPot</name><description>[0/4.34]? Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>loggf</name><description>[-9.82/0.76]? Log oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_EW</name><description>Flag on EW (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>EW</name><description>[6.78/162]? Equivalent width</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_logeps(x)</name><description>Limit flag on logeps</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logeps(x)</name><description>[-2.85/7.36] Log number abundance of Ion</description><unit>log(Sun)</unit><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>