J/ApJ/711/619ivo://CDS.VizieR/J/ApJ/711/619doi:10.26093/cds/vizier.17110619CDSMilingo J.B.Kwitter K.B.Henry R.B.C.Souza S.P.2017-12-12T14:45:07Z2012-04-23T14:05:34ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frchemical-abundancesplanetary-nebulaespectroscopymilky-way-galaxyIn this paper, we present emission line strengths, abundances, and element ratios (X/O for Ne, S, Cl, and Ar) for a sample of 38 Galactic disk planetary nebulae (PNe) consisting primarily of Peimbert classification Type I. Spectrophotometry for these PNe incorporates an extended optical/near-IR range of 3600-9600{AA} including the [SIII] lines at 9069{AA} and 9532{AA}, setting this relatively large sample apart from typical spectral coverage. We have utilized Emission Line Spectrum Analyzer, a five-level atom abundance routine, to determine Te, Ne, ionization correction factors, and total element abundances, thereby continuing our work toward a uniformly processed set of data. With a compilation of data from >120 Milky Way PNe, we present results from our most recent analysis of abundance patterns in Galactic disk PNe. With a wide range of metallicities, galactocentric distances, and both Type I and non-Type I objects, we have examined the alpha elements against HII regions and blue compact galaxies (H2BCGs) to discern signatures of depletion or enhancement in PNe progenitor stars, particularly the destruction or production of O and Ne.2010ApJ...711..619Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/711/619CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/500/1089 : Abundances in planetary nebulae (Gorny+, 2009)J/A+A/494/591 : Abundances in planetary nebulae (Chiappini+, 2009)J/PAZh/35/574 : He, C, N and O abundances in planetary nebulae (Milanova+,J/AZh/82/437 : Calculated chemical composition of galactic PN (Holovatyy+,J/MNRAS/349/793 : Galactic PNe abundances (Perinotto+, 2004)J/A+A/427/231 : Abundances in planetary nebulae (Gorny+, 2004)J/A+A/423/199 : Chemical abundances of planetary nebulae (Costa+, 2004)J/A+A/380/300 : Abundances of PN towards Galactic bulge (Escudero+, 2001)J/A+A/345/629 : Abundance gradients in planetary nebulae (Maciel+, 1999)J/A+AS/126/297 : PN abundances (Ratag+ 1997)J/A+A/280/581 : Chemical abundances of PNe (Pasquali+, 1993)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/711/619https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/711/619http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/711/619https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/711/619https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/711/619http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/711/619GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/711/619/pne (Extinction measures and H{beta} flux for each PN)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/711/619/pne?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/711/619/pne?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/711/619/pne?GETtext/xml+votable180.050000true274.392110.15092780.0055555555555555566/2979 12983 13968 14118 14642 15552 15621 15639 15739 20829 21600 21732 22226 22660 28780 28906 28917 28923 29096 29213 29255 29267 29886 30288 30308 30527 30656 30686 31847 38075 39775 39801 39860 41574 41768 42147 42168 42446https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/711/619?format=asciiOpticaldefaultJ/ApJ/711/619/pneExtinction measures and H{beta} flux for each PNSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePN namemeta.id;meta.maincharprimarycExtinction measure (G1)obs.atmos.extinctionfloatHa/HbFinal converged H{alpha}/H{beta} line ratiophys.atmol.final;arith.ratio;spect.linefloatlog(FHb)Log of the observed H{beta} flux in units of erg/s/cm^2^log(mW.m**-2)phot.flux;em.line.Hbeta;arith.ratiofloat_RAPositions from SIMBAD database (right ascension part)degpos.eq.ra;meta.main_DEPositions from SIMBAD database (declination part)degpos.eq.dec;meta.mainJ/ApJ/711/619/table2Fluxes and intensitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePlanetary nebula identificationmeta.id;meta.maincharLineIDLine identificationmeta.id;spect.linelambdaWavelength ({AA})0.1nmem.wlintn_lambda[a] deblended linemeta.notecharf(lam)Reddening function (G1)phot.color.excessfloatF(lam)? Raw, uncorrected line flux (3)phot.flux;arith.ratiodoublenullablef_F(lam)Uncertainty flag on F(lam) (4)meta.codecharI(lam)? Dereddened line flux (3)spect.line.intensity;arith.ratiodoublenullablee_I(lam)? Uncertainty in I(lam) (3)stat.errordoublenullableu_I(lam)Uncertainty flag on I(lam) (4)meta.code.errorcharJ/ApJ/711/619/table3Temperatures and densitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePlanetary nebula identificationmeta.id;meta.maincharParamParameter (1)meta.noteValue? Parameter value (2)stat.paramintnullablee_Value? Uncertainty in Valuestat.error;stat.valueintnullablen_ValueNote on Value (3)meta.notecharJ/ApJ/711/619/table4Ionic abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePlanetary nebula identificationmeta.id;meta.maincharIonIon or icf (ionization correction factors)phys.atmol.ionStageTmethMethod used to determine the temperature (1)meta.notecharf_Abd[*] Indicates Abd included in weighted meanmeta.codecharAbd? Derived ionic abundance or icfphys.abunddoublenullablee_Abd? Uncertainty in Abdstat.errordoublenullableJ/ApJ/711/619/table5Total elemental abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNamePlanetary nebula identificationmeta.id;meta.maincharRatioIons concernedmeta.notecharAbd? Abundance ratio (1)phys.abunddoublenullablee_Abd? Uncertainty in Abd (1)stat.errordoublenullableSolarAsplund et al., 2005ASPC..336...25A, solar abundance ratio (1)phys.abunddoubleOrionEsteban et al., 1998MNRAS.295..401E, Orion abundance ratio (1)phys.abunddouble