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<ri:Resource created="2022-02-15T14:10:15Z" 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>Variability in protoplanetary nebulae. VII. 5 LCs</title><shortName>J/ApJ/901/9</shortName><identifier>ivo://CDS.VizieR/J/ApJ/901/9</identifier><altIdentifier>doi:10.26093/cds/vizier.19010009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hrivnak B.J.</name></creator><creator><name>Henson G.</name></creator><creator><name>Hillwig T.C.</name></creator><creator><name>Lu W.</name></creator><creator><name>Nault K.A.</name></creator><creator><name>Volk K.</name></creator><date role="Updated">2024-10-25T20:14:01Z</date><date role="Created">2022-02-15T14:10:15Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>stellar-spectral-types</subject><description>We have monitored over a 10-year interval the light variations of five evolved stars with very large mid-infrared excesses. All five objects appear to have oxygen-rich or mixed oxygen-rich and carbon-rich chemistries. They all vary in light: four over a small range of ~0.2mag and the fifth over a larger range of ~0.7mag. Spectral types range from G2 to B0. Periodic pulsations are found for the first time in the three cooler ones, IRAS18075-0924 (123d), 19207+2023 (96d), and 20136+1309 (142d). No significant periodicity is found in the hotter ones, but they appear to vary on a shorter timescale of a few days or less. Two also show some evidence of longer-term periodic variations (~4yr). Three appear to be protoplanetary nebulae (PPNe), in the post-asymptotic giant branch (post-AGB) phase of stellar evolution. Their light variations are in general agreement with the relationships among temperature, pulsation period, and pulsation amplitude found in previously studied PPNe. The other two, however, appear to have too low a luminosity (1000-1500L_{sun}_), based on Gaia distances, to be in the post-AGB phase. Instead, they appear to be Milky Way analogs of the recently identified class of dusty post-red giant branch (post-RGB) stars found in the Magellanic Clouds, which likely had their evolution interrupted by interaction with a binary companion. If this is the case, then these would be among the first dusty post-RGB objects identified in the the Milky Way.</description><source format="bibcode">2020ApJ...901....9H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/901/9</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/II/118">II/118 : UBVRI standards around Celestial Equator (Landolt 1983)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/125">II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/183">II/183 : UBVRI Photometric Standards (Landolt 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/305">I/305 : The Guide Star Catalog, Version 2.3.2 (GSC2.3) (STScI, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</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/A+A/299/755">J/A+A/299/755 : Stellar evolution. II. Post-AGB (Bloecker+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/458/173">J/A+A/458/173 : Optical spectroscopy of 253 IRAS sources (Suarez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/36/281">J/PAZh/36/281 : Variability of 3 protoplanetary nebulae (Arkhipova+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1042">J/ApJ/709/1042 : Variability in C-rich proto-PNe. (Hrivnak+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/766/116">J/ApJ/766/116 : Variability in proto-PNe. II. (Hrivnak+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/439/2211">J/MNRAS/439/2211 : Post-AGB/RGB and YSOs in SMC (Kamath+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/794/81">J/ApJ/794/81 : Maser and IR studies of oxygen-rich AGB stars (Yung+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/149/184">J/AJ/149/184 : Long-term photometry for 4 O-rich PPne (Hrivnak+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/454/1468">J/MNRAS/454/1468 : LMC post-AGB, post-RGB star and YSOs (Kamath+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/447/1673">J/MNRAS/447/1673 : Galactic post-AGB stars distances (Vickers+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/588/A25">J/A+A/588/A25 : Post-AGB &amp; CSPNe models (Miller Bertolami, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/826/44">J/ApJ/826/44 : Spitzer/IRS obs. of Magellanic carbon stars (Sloan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/300">J/AJ/156/300 : Velocity and LC analysis of three PPNe (Hrivnak+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/21">J/AJ/159/21 : V and Rc light curves of medium-bright PPNe (Hrivnak+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/649/A164">J/A+A/649/A164 : Protoplanetary nebulae &amp; young PN CO sp. 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