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<ri:Resource created="2019-05-09T14:02:02Z" 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>Velocity and light curve analysis of three PPNe</title><shortName>J/AJ/156/300</shortName><identifier>ivo://CDS.VizieR/J/AJ/156/300</identifier><altIdentifier>doi:10.26093/cds/vizier.51560300</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hrivnak B.J.</name></creator><creator><name>Van de Steene G.</name></creator><creator><name>Van Winckel H.</name></creator><creator><name>Lu W.</name></creator><creator><name>Sperauskas J.</name></creator><date role="Updated">2024-10-25T20:12:01Z</date><date role="Created">2019-05-09T14:02:02Z</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>giant-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>radial-velocity</subject><subject>stellar-spectral-types</subject><subject>effective-temperature</subject><subject>chemical-abundances</subject><description>We have obtained contemporaneous light, color, and radial velocity data for three proto-planetary nebulae (PPNe) over the years 2007 to 2015. The light and velocity curves of each show similar periods of pulsation, with photometric periods of 42 and 50 days for IRAS 17436+5003, 102 days for IRAS 18095+2704, and 35 days for IRAS 19475+3119. The light and velocity curves are complex with multiple periods and small, variable amplitudes. Nevertheless, at least over limited time intervals, we were able to identify dominant periods in the light, color, and velocity curves and compare the phasing of each. The color curves appear to peak with or slightly after the light curves while the radial velocity curves peak about a quarter of a cycle before the light curves. Similar results were found previously for two other PPNe, although for them the light and color appeared to be in phase. Thus, it appears that PPNe are brightest when smallest and hottest. These phase results differ from those found for classical Cepheid variables, where the light and velocity differ by half a cycle, and are hottest at about average size and expanding. However, they do appear to have similar phasing to the larger-amplitude pulsations seen in RV Tauri variables. Presently, few pulsation models exist for PPNe, and these do not fit the observations well, especially the longer periods observed. Model fits to these new light and velocity curves would allow masses to be determined for these post-AGB objects, and thereby provide important constraints to post-AGB stellar evolution models of low- and intermediate-mass stars.</description><source format="bibcode">2018AJ....156..300H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/300</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+AS/126/479">J/A+AS/126/479 : NIR photometry of IRAS sources. III (Garcia-Lario+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/122/221">J/ApJS/122/221 : A mid-IR survey of Proto-PNs Candidates (Meixner+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/250">J/A+A/368/250 : Abundances of HDE 341617 (Arellano Ferro+, 2001)</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/PASJ/59/1127">J/PASJ/59/1127 : Abundances in 5 post-AGB candidates (Takeda+, 2007)</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/PAZh/36/281">J/PAZh/36/281 : Variability of 3 protoplanetary nebulae (Arkhipova+, 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/AJ/149/184">J/AJ/149/184 : Long-term photometry for 4 O-rich PPne (Hrivnak+, 2015)</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/AJ/156/300</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/300</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/300</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/300</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/300</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/156/300</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/156/300/table1 (Program objects)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/156/300/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/156/300/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/156/300/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>266.2311233</ra><dec>50.0443011</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/9713 14450 32543</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/156/300?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/156/300/table1</name><description>Program objects</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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