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<ri:Resource created="2023-02-01T08:44:57Z" 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>Abundances in extincted Milky Way planetary nebulae</title><shortName>J/AJ/164/185</shortName><identifier>ivo://CDS.VizieR/J/AJ/164/185</identifier><altIdentifier>doi:10.26093/cds/vizier.51640185</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Manea C.</name></creator><creator><name>Dinerstein H.L.</name></creator><creator><name>Sterling N.C.</name></creator><creator><name>Zeimann G.</name></creator><date role="Updated">2023-02-15T07:43:59Z</date><date role="Created">2023-02-01T08:44:57Z</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><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><subject>astrometry</subject><subject>radial-velocity</subject><description>Low- and intermediate-mass (0.8M{sun}&lt;M&lt;8M{sun}) stars that evolve into planetary nebulae (PNe) play an important role in tracing and driving Galactic chemical evolution. Spectroscopy of PNe enables access to both the initial composition of their progenitor stars and products of their internal nucleosynthesis, but determining accurate ionic and elemental abundances of PNe requires high-quality optical spectra. We obtained new optical spectra of eight highly-extincted PNe with limited optical data in the literature using the Low Resolution Spectrograph 2 on the Hobby-Eberly Telescope. Extinction coefficients, electron temperatures and densities, and ionic and elemental abundances of up to 11 elements (He, N, O, Ne, S, Cl, Ar, K, Fe, Kr, and Xe) are determined for each object in our sample. Where available, astrometric data from Gaia EDR3 is used to kinematically characterize the probability that each object belongs to the Milky Way's thin disk, thick disk, or halo. Four of the PNe show kinematic and chemical signs of thin disk membership, while two may be members of the thick disk. The remaining two targets lack Gaia data, but their solar O, Ar, and Cl abundances suggest thin disk membership. Additionally, we report the detection of broad emission features from the central star of M3-35. Our results significantly improve the available information on the nebular parameters and chemical compositions of these objects, which can inform future analyses.</description><source format="bibcode">2022AJ....164..185M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/164/185</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><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/64">VI/64 : Recombination line intensities for hydrogenic ions (Storey+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VI/141">VI/141 : Nebular [OIII] collision strengths - SSB (Storey+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/116/573">J/A+AS/116/573 : Transitions for FeIII (Quinet 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/123/159">J/A+AS/123/159 : IRON Project. XXII. C and O radiative rates (Galavis+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/526/544">J/ApJ/526/544 : Collision strengths in S III (Tayal+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/387/1135">J/A+A/387/1135 : NII effective recombination coefficients (Kisielius+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/403/659">J/A+A/403/659 : Classification of WR planetary nebulae (Acker+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/410/527">J/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/426/717">J/A+A/426/717 : Oscillator strengths for ClII lines (Tayal+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/463/265">J/A+A/463/265 : Chemical comp. of 48 WR planetary nebulae (Girard+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/1265">J/ApJ/659/1265 : Emission lines in 4 planetary nebulae (Sharpee+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/32">J/ApJS/188/32 : Breit-Pauli transition probabilities for SII (Tayal+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/415/181">J/MNRAS/415/181 : Deep spectroscopy of NGC 7009 (Fang+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/130">J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/2606">J/MNRAS/452/2606 : Deep echelle spectro. of NGC3918 (Garcia-Rojas+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/25">J/ApJS/218/25 : Abundances in PNe. 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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>Target name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>PNG</name><description>Target PNG identifier (PN GLLL.l+BB.b)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Diam</name><description>[2/18.6] Optical diameters (1)</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>CSType</name><description>Central Star Type (mag) (2)</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>f_CSType</name><description>[*] Although not previously reported in the litterature, M3-35 displays weak stellar wind lines</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Obs</name><description>[2020] Year of observation</description><ucd>time.epoch</ucd></column><column><name>Texp-L</name><description>[370/2674] Exposure time (long)</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Texp-S</name><description>[30/120] Exposure time (short)</description><unit>s</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Note</name><description>Observing notes</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>Pos</name><description>RVel, Dist, galactic positions (table5)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>_RA</name><description>Position from SIMBAD (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from SIMBAD (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/AJ/164/185/table5</name><description>Radial velocities, distances, galactic positions</description><column><name>e_Z</name><description>[0/0.2] Error on Z</description><unit>kpc</unit><ucd>stat.error;src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Name</name><description>Target name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>e_U</name><description>[5/43] Error on U</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></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>RVel</name><description>[-189/107] Radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_RVel</name><description>[10/12] Error on RVel</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>[1.67/6.24] Distance</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Dist</name><description>[0.1/3] Negative error on Dist</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Dist</name><description>[0.2/3] Positive error on Dist</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>X</name><description>[4.47/12.5] Galactocentric X position</description><unit>kpc</unit><ucd>pos.cartesian.x;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_X</name><description>[0.06/2] Error on X</description><unit>kpc</unit><ucd>stat.error;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Y</name><description>[1.55/5.92] Galactocentric Y position</description><unit>kpc</unit><ucd>pos.cartesian.y;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Y</name><description>[0.1/2] Error on Y</description><unit>kpc</unit><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Z</name><description>[-0.24/0.72] Galactocentric Z position</description><unit>kpc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>U</name><description>[37.6/188] Galactrocentric U velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>V</name><description>[-214/-32] Galactocentric V velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_V</name><description>[6/60] Error on V</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W</name><description>[-50/1.5] Galactocentric W velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_W</name><description>[1/24] Error on W</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/164/185/tablea1</name><description>Observed fluxes</description><column><name>M2-43</name><description>[0.01/2616]? 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