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<ri:Resource created="2021-08-04T14:24:39Z" 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>Galactic planetary nebulae with Gaia data</title><shortName>J/ApJ/889/21</shortName><identifier>ivo://CDS.VizieR/J/ApJ/889/21</identifier><altIdentifier>doi:10.26093/cds/vizier.18890021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stanghellini L.</name></creator><creator><name>Bucciarelli B.</name></creator><creator><name>Lattanzi M.G.</name></creator><creator><name>Morbidelli R.</name></creator><date role="Updated">2022-07-07T17:53:23Z</date><date role="Created">2021-08-04T14:24:39Z</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>planetary-nebulae</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><description>We matched the astrometry of central stars (CSs) of spectroscopically confirmed Galactic planetary nebulae (PNe) with DR2 Gaia parallaxes (p), finding 430 targets in common with p&gt;0 and |{sigma}_p_/p|&lt;1. A catalog of PNe whose CSs have DR2 Gaia parallaxes is presented in Table 1. We compared DR2 parallaxes with those in the literature, finding good correlation between the two samples. We used PNe parallaxes to calibrate the Galactic PN distance scale. Restricting the sample to objects with 20% parallax accuracy, we derive the distance scale log(R_pc_)=-(0.226+/-0.0155)xlog(S_H{beta}_)-(3.920+/-0.215), which represents a notable improvement with respect to previous ones. We found that the ionized mass versus optical thickness distance scale for Galactic PNe is not as constrained by the Gaia calibrators, but gives important insight into the nature of the PNe, and is essential to define the domain for our distance scale application. We placed the CSs whose distance has been determined directly by parallax on the HR diagram, and found that their location on the post-asymptotic-giant-branch (AGB) H-burning evolutionary tracks is typical for post-AGB stars.</description><source format="bibcode">2020ApJ...889...21S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/889/21</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/V/84">V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/94/399">J/A+AS/94/399 : Absolute fluxes and distances of PN (Cahn+, 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/92/125">J/ApJS/92/125 : Post-AGB evolution (Vassiliadis+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/459/606">J/ApJ/459/606 : Distances of planetary nebulae (Schneider+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/405/627">J/A+A/405/627 : Angular dimensions of 312 planetary nebulae (Tylenda+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/408/1029">J/A+A/408/1029 : Coordinates of Galactic planetary nebulae (Kerber+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/689/194">J/ApJ/689/194 : Distances of galactic planetary nebulae (Stanghellini+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A25">J/A+A/588/A25 : Post-AGB &amp; CSPNe evolutionary models (Miller Bertolami, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A10">J/A+A/616/A10 : 46 open clusters GaiaDR2 HR diag (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/L2">J/A+A/616/L2 : Planetary Nebulae distances in Gaia DR2 (Kimeswenger+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/630/A150">J/A+A/630/A150 : Astrometric data for 211 GAPN (Gonzalez-Santamaria+, 2019)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/889/21</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/889/21</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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