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<ri:Resource created="2026-06-12T13:55:32Z" status="active" updated="2026-06-20T14:48:47Z" 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>Study of TESS LCs RRc stars variation modes</title><shortName>J/MNRAS/521/443</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/521/443</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Benko J.M.</name></creator><creator><name>Plachy E.</name></creator><creator><name>Netzel H.</name></creator><creator><name>Bodi A.</name></creator><creator><name>Molnar L.</name></creator><creator><name>Pal A.</name></creator><date role="Updated">2026-06-20T14:48:47Z</date><date role="Created">2026-06-12T13:55:32Z</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>variable-stars</subject><subject>asteroseismology</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Using two years of data from the TESS space telescope, we have investigated the time series of 633 overtone pulsating field RR Lyrae (RRc) stars. The majority of stars (82.8 per cent) contain additional frequencies beyond the main pulsation. In addition to the frequencies previously explained by the l = 8 and 9 non-radial modes, we have identified a group of stars where the additional frequencies may belong to the l = 10 non-radial modes. We found that stars with no additional frequencies are more common among stars with shorter periods, while stars with longer periods almost always show additional frequencies. The incidence rate and this period distribution both agree well with the predictions of recent theoretical models. The amplitude and phase of additional frequencies are varying in time. The frequencies of different non-radial modes appearing in a given star seem to vary on different time-scales. We have determined a 10.4 per cent incidence rate for the Blazhko effect. For several stars we have detected continuous annual-scale phase change without significant amplitude variation. This type of variation offers a plausible explanation for the 'phase jump' phenomenon reported in many RRc stars. The main pulsation frequency could show quasi-periodic phase and amplitude fluctuations. This fluctuation is clearly related to additional frequencies present in the star: stars with two non-radial modes show the strongest fluctuations, while stars with no such modes show no fluctuations at all. The summation of the phase fluctuation over time may explain the O-C variations that have long been known for many non-Blazhko RRc stars.</description><source format="bibcode">2023MNRAS.521..443B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/521/443</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/MNRAS/491/4752">J/MNRAS/491/4752 : Modelled parameters of Cepheid and RR Lyrae</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/487/5584">J/MNRAS/487/5584 : First-overtone RR Lyrae stars from OGLE (Netzel+, 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ivo-id="ivo://CDS.VizieR/J/A+A/476/307">J/A+A/476/307 : Period variations in galactic RRab stars (Le Borgne+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/258/8">J/ApJS/258/8 : LCs of RR Lyrae stars from TESS (Molnar+, 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/253/11">J/ApJS/253/11 : TESS observations of Cepheid stars (Plachy+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/244/32">J/ApJS/244/32 : Extended Aperture Photometry of K2 RR Lyrae stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/213/31">J/ApJS/213/31 : Blazhko effect from 4yr of Kepler data (Benko+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/69/321">J/AcA/69/321 : OGLE RR Lyrae stars in Galactic bulge and disk</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/66/131">J/AcA/66/131 : VI light curves of SMC and LMC RR Lyrae (Soszynski+, 2016)</relatedResource><relatedResource 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