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<ri:Resource created="2022-09-02T13:30:47Z" 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 post-AGB stars in Gaia DR3</title><shortName>J/MNRAS/516/L61</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/516/L61</identifier><altIdentifier>doi:10.26093/cds/vizier.75169061</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Oudmaijer R.D.</name></creator><creator><name>Jones E.R.M.</name></creator><creator><name>Vioque M.</name></creator><date role="Updated">2024-08-22T20:16:21Z</date><date role="Created">2022-09-02T13:30:47Z</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>giant-stars</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>stellar-distance</subject><subject>effective-temperature</subject><description>This paper presents the first census of Galactic post-asymptotic Giant Branch stars in the HR diagram. We combined Gaia DR3 parallax-based distances with extinction corrected integrated fluxes, and derived luminosities for a sample of 185 stars that had been proposed to be post-AGB stars in the literature. The luminosities allow us to create an HR diagram containing the largest number of post-AGB candidate objects to date. A significant fraction of the objects fall outside the typical luminosity range as covered by theoretical evolutionary post-AGB tracks as well as observed for Planetary Nebula central stars. These include massive evolved supergiants and lower luminosity objects. Here we highlight the fact that one third of the post-AGB candidates is underluminous and we identify these with the recently recognised class of post-Red Giant Branch objects thought to be the result of binary evolution.</description><source format="bibcode">2022MNRAS.516L..61O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/516/L61</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/J/A+A/469/799">J/A+A/469/799 : Torun catalog of post-AGB &amp; related objects (Szczerba+ 2007)</relatedResource><relatedResource 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