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<ri:Resource created="2014-12-12T08:32:13Z" 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 proto-PNe. II.</title><shortName>J/ApJ/766/116</shortName><identifier>ivo://CDS.VizieR/J/ApJ/766/116</identifier><altIdentifier>doi:10.26093/cds/vizier.17660116</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hrivnak B.J.</name></creator><creator><name>Lu W.</name></creator><creator><name>Sperauskas J.</name></creator><creator><name>Van Winckel H.</name></creator><creator><name>Bohlender D.</name></creator><creator><name>Zacs L.</name></creator><date role="Updated">2024-10-25T20:13:46Z</date><date role="Created">2014-12-12T08:32:13Z</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>carbon-stars</subject><subject>planetary-nebulae</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>radial-velocity</subject><description>We have carried out a detailed observational study of the light, color, and velocity variations of two bright, carbon-rich proto-planetary nebulae, IRAS 22223+4327 and 22272+5435. The light curves are based upon our observations from 1994 to 2011, together with published data by Arkhipova and collaborators. They each display four significant periods, with primary periods for IRAS 22223+4327 and 22272+5435 being 90 and 132 days, respectively. For each of them, the ratio of secondary to primary period is 0.95, a value much different from that found in Cepheids, but which may be characteristic of post-asymptotic giant branch (AGB) stars. Fewer significant periods are found in the smaller radial velocity data sets, but they agree with those of the light curves. The color curves generally mimic the light curves, with the objects reddest when faintest. A comparison in seasons when there exist contemporaneous light, color, and velocity curves reveals that the light and color curves are in phase, while the radial velocity curves are ~0.25 P out of phase with the light curves. Thus they differ from what is seen in Cepheids, in which the radial velocity curve is 0.50 P out of phase with the light curve. Comparison of the observed periods and amplitudes with those of post-AGB pulsation models shows poor agreement, especially for the periods, which are much longer than predicted. These observational data, particularly the contemporaneous light, color, and velocity curves, provide an excellent benchmark for new pulsation models of cool stars in the post-AGB, proto-planetary nebula phase.</description><source format="bibcode">2013ApJ...766..116H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/766/116</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/ApJS/211/15">J/ApJS/211/15 : SiO &amp; H2O maser survey toward AGB+post-AGB stars (Yoon+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/37/691">J/PAZh/37/691 : V340 Ser and V448 Lac light curves (Arkhipova+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/88/34">J/AZh/88/34 : Long-term (1984-2008) JHKLM phot. of stars (Shenavrin+, 2011)</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/other/PZ/29.1">J/other/PZ/29.1 : UBV light curves of V354 Lac (Arkhipova+, 2009)</relatedResource><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 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/A+A/431/565">J/A+A/431/565 : Evolved stars in the MSX survey (Ortiz+, 2005)</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/A+A/323/469">J/A+A/323/469 : Optical spectra of post-AGB stars (Bakker+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/299/755">J/A+A/299/755 : Stellar evolution. II. 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