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<ri:Resource created="2024-05-02T14:43:36Z" status="active" updated="2025-06-13T15:25:00Z" 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>PN chemical abundances in Galactic Bulge</title><shortName>J/MNRAS/527/6363</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/527/6363</identifier><altIdentifier>doi:10.26093/cds/vizier.75276363</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tan S.</name></creator><creator><name>Parker Q.A.</name></creator><creator><name>Zijlstra A.A.</name></creator><creator><name>Rees B.</name></creator><date role="Updated">2024-11-06T20:35:06Z</date><date role="Created">2024-05-02T14:43:36Z</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>milky-way-galaxy</subject><subject>planetary-nebulae</subject><subject>chemical-abundances</subject><description>In this, the third of a series of papers, we present well determined chemical abundances for 124 Planetary nebulae (PNe) in the Galactic bulge from deep, long-slit FORS2 spectra from the 8.2 m ESO Very Large telescope (VLT). Prior to this work there were only ~240 bulge PNe with chemical abundances previously determined over a ~50 year period and of highly variable quality. For 34 of these PNe we are presenting their abundances for the first time which adds ~14% to the available sample of bulge PNe abundances. The interstellar reddening, physical conditions (electron densities, ne, temperatures, Te), and chemical compositions are derived as single values for each PN but also using different line diagnostics. 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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>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>n_PNG</name><description>[*] * when PN has an abundance determined for the first time</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>PNG</name><description>PNG name (LLL.l+BB.b)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>c(Hb)</name><description>logarithmic interstellar extinction c at H{beta} derived from our spectra</description><ucd>phys.absorption.coeff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_c(Hb)</name><description>Error on c(Hb) (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_c(Hb)</name><description>Error on c(Hb) (lower value)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>He/H</name><description>? Abundance for the He/H ratio on a scale such that log(H)=12</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_He/H</name><description>? Error on He/H (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_He/H</name><description>? Error on He/H (lower value)</description><ucd>stat.error;phys.abund.Y</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N/H</name><description>? Abundance for the N/H ratio on a scale such that log(H)=12</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_N/H</name><description>? Error on N/H (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_N/H</name><description>? Error on N/H (lower value)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>O/H</name><description>Abundance for the O/H ratio on a scale such that log(H)=12</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_O/H</name><description>? Error on O/H (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_O/H</name><description>? Error on O/H (lower value)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ne/H</name><description>? Abundance for the Ne/H ratio on a scale such that log(H)=12</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_Ne/H</name><description>? Error on Ne/H (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ne/H</name><description>? Error on Ne/H (lower value)</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S/H</name><description>Abundance for the S/H ratio on a scale such that log(H)=12</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_S/H</name><description>? Error on S/H (upper value)</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_S/H</name><description>? 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Uncertainty in the intensity of [SIII] 6312A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(6548)</name><description>Uncertainty in the intensity of [NII] 6548A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_I(6563)</name><description>Uncertainty in the intensity of HI 6563A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_I(6584)</name><description>Uncertainty in the intensity of [NII] 6584A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_I(6678)</name><description>? Uncertainty in the intensity of HeI 6678A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(6716)</name><description>Uncertainty in the intensity of [SII] 6716A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_I(6731)</name><description>Uncertainty in the intensity of [SII] 6731A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_I(7006)</name><description>? Uncertainty in the intensity of [ArV] 7006A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(7136)</name><description>? Uncertainty in the intensity of [ArIII] 7136A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(7319)</name><description>? Uncertainty in the intensity of [OII] 7319A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(7330)</name><description>? Uncertainty in the intensity of [OII] 7330A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(7531)</name><description>? Uncertainty in the intensity of [ClIV] 7531A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(7751)</name><description>? Uncertainty in the intensity of [ArIII] 7751A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_I(8046)</name><description>? Uncertainty in the intensity of [ClIV] 8046A line</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>