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<ri:Resource created="2012-04-02T12:09:32Z" 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 C-rich proto-PNe.</title><shortName>J/ApJ/709/1042</shortName><identifier>ivo://CDS.VizieR/J/ApJ/709/1042</identifier><altIdentifier>doi:10.26093/cds/vizier.17091042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hrivnak B.J.</name></creator><creator><name>Lu W.</name></creator><creator><name>Maupin R.E.</name></creator><creator><name>Spitzbart B.D.</name></creator><date role="Updated">2024-10-25T20:13:40Z</date><date role="Created">2012-04-02T12:09:32Z</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>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>effective-temperature</subject><subject>planetary-nebulae</subject><subject>giant-stars</subject><subject>carbon-stars</subject><description>We have carried out long-term (14 years) V and R photometric monitoring of 12 carbon-rich proto-planetary nebulae. The light and color curves display variability in all of them. The light curves are complex and suggest multiple periods, changing periods, and/or changing amplitudes, which are attributed to pulsation. A dominant period has been determined for each and found to be in the range of ~150 days for the coolest (G8) to 35-40 days for the warmest (F3). A clear, linear inverse relationship has been found in the sample between the pulsation period and the effective temperature and also an inverse relationship between the amplitude of light variation and the effective temperature. These are consistent with the expectation for a pulsating post-asymptotic giant branch (post-AGB) star evolving toward higher temperature at constant luminosity. The published spectral energy distributions and mid-infrared images show these objects to have cool (200K), detached dust shells and published models imply that intensive mass loss ended 400-2000 years ago.</description><source format="bibcode">2010ApJ...709.1042H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/709/1042</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</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/254">I/254 : The HST Guide Star Catalog, Version 1.2 (Lasker+ 1996)</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/J/A+A/369/178">J/A+A/369/178 : Effective temperatures of carbon-rich stars (Bergeat+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/26/705">J/PAZh/26/705 : UBV observations of post-AGB supergiants (Arkhipova+, 2000)</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+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/A+A/267/515">J/A+A/267/515 : Very cold C-rich circumstellar envelopes (Omont+ 1993)</relatedResource><relatedResource>http://www.iac.es/proyecto/apn4/pages/proceedings.php : Asymmetrical PNe IV</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/709/1042</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/709/1042</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/709/1042</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/709/1042</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/709/1042</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/709/1042</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/ApJ/709/1042/ppne (List of C-rich proto-PNe observed)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/709/1042/ppne?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/709/1042/ppne?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/709/1042/ppne?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>36.674167</ra><dec>62.356111</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1229 3649 13297 13917 14256 14323 14453 22392 22425 23695 24079 48822</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/ApJ/709/1042?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/709/1042/ppne</name><description>List of C-rich proto-PNe observed</description><column><name>2M</name><description>Display the 2MASS data (Cutri et al. 2003, Cat. 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Detection of C_3_ absorption</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>AIBs</name><description>[Y] Aromatic infrared bands (AIBs) in emission at 3.3, 6.2, 7.7, 8.6, and 11.3um</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>f_AIBs</name><description>[b] b: Weak plateau features</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>21um</name><description>[Y] Broad emission feature at 20.1um</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>30um</name><description>[Y] Very broad emission feature around 30um</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>SpT</name><description>MK spectral type</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column></table><table><name>J/ApJ/709/1042/table3</name><description>Magnitudes of the PPNs on the standard BVRI system at the time of the observations</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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