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<ri:Resource created="2022-12-15T12:41:08Z" 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>Chemical compositions of Galactic bulge stars</title><shortName>J/MNRAS/486/5349</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/486/5349</identifier><altIdentifier>doi:10.26093/cds/vizier.74865349</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Duong L.</name></creator><creator><name>Asplund M.</name></creator><creator><name>Nataf D.M.</name></creator><creator><name>Freeman K.C.</name></creator><creator><name>Ness M.</name></creator><date role="Updated">2024-08-19T20:18:35Z</date><date role="Created">2022-12-15T12:41:08Z</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>milky-way-galaxy</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>infrared-astronomy</subject><description>This work explores the detailed chemistry of the Milky Way bulge using the HERMES spectrograph on the Anglo-Australian Telescope. Here, we present the abundance ratios of 13 elements for 832 red giant branch and clump stars along the minor bulge axis at latitudes b=-10{deg},-7.5{deg}, and -5{deg}. Our results show that none of the abundance ratios vary significantly with latitude. We also observe disc-like [Na/Fe] abundance ratios, which indicate that the bulge does not contain helium-enhanced populations as observed in some globular clusters. Helium enhancement is therefore not the likely explanation for the double red-clump observed in the bulge. We confirm that bulge stars mostly follow abundance trends observed in the disc. However, this similarity is not confirmed across all elements and metallicity regimes. The more metal-poor bulge population at [Fe/H]~&lt;-0.8 is enhanced in the elements associated with core collapse supernovae (SNeII). In addition, the [La/Eu] abundance ratio suggests higher r-process contribution, and likely higher star formation in the bulge compared to the disc. 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Zr to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Zr/Fe]</name><description>? Error on [Zr/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[La/Fe]</name><description>? La to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[La/Fe]</name><description>? Error on [La/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Ce/Fe]</name><description>? Ce to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/486/5349/tableb1c</name><description>Abundances catalogue for 300 red giant branch and clump stars along the minor bulge axis at latitude b=-10{deg}</description><column><name>e_[Ni/Fe]</name><description>? Error on [Ni/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></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>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>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Teff</name><description>Error on Teff</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">double</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">double</dataType></column><column><name>e_logg</name><description>Error on logg</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</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">double</dataType></column><column><name>e_[Fe/H]</name><description>Error on [Fe/H]</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>[Na/Fe]</name><description>? Na to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Na/Fe]</name><description>? Error on [Na/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Al/Fe]</name><description>? Al to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Al/Fe]</name><description>? Error on [Al/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Sc/Fe]</name><description>? Sc to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Sc/Fe]</name><description>? Error on [Sc/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Cr/Fe]</name><description>? Cr to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Cr/Fe]</name><description>? Error on [Cr/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Mn/Fe]</name><description>? Mn to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Mn/Fe]</name><description>? Error on [Mn/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Co/Fe]</name><description>? Co to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Co/Fe]</name><description>? Error on [Co/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></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>[Ni/Fe]</name><description>? Ni to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Cu/Fe]</name><description>? Cu to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Cu/Fe]</name><description>? Error on [Cu/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Zr/Fe]</name><description>? Zr to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Zr/Fe]</name><description>? Error on [Zr/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[La/Fe]</name><description>? La to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[La/Fe]</name><description>? Error on [La/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Ce/Fe]</name><description>? Ce to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Ce/Fe]</name><description>? Error on [Ce/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Nd/Fe]</name><description>? Nd to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Nd/Fe]</name><description>? Error on [Nd/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>[Eu/Fe]</name><description>? Eu to iron abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_[Eu/Fe]</name><description>? Error on [Eu/Fe]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>ID</name><description>2MASS source identifier (HHMMSSSS+DDMMSSS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column></table><table><name>J/MNRAS/486/5349/tableb2</name><description>Lines and atomic data used to derive abundance ratios in this work</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>Species</name><description>Lines used to derive abundance ratios</description><ucd>meta.id;spect.line</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>lambda</name><description>Wavelenght ({AA})</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>loggf</name><description>Logarithm of oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EP</name><description>Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>