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<ri:Resource created="2018-11-27T12:29:57Z" 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>Dissipation in exoplanet hosts from tidal spin-up</title><shortName>J/AJ/155/165</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/165</identifier><altIdentifier>doi:10.26093/cds/vizier.51550165</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Penev K.</name></creator><creator><name>Bouma L.G.</name></creator><creator><name>Winn J.N.</name></creator><creator><name>Hartman J.D.</name></creator><date role="Updated">2019-01-07T09:02:13Z</date><date role="Created">2018-11-27T12:29:57Z</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>multiple-stars</subject><subject>exoplanets</subject><subject>stellar-masses</subject><subject>stellar-radii</subject><subject>astronomical-models</subject><description>Stars with hot Jupiters (HJs) tend to rotate faster than other stars of the same age and mass. This trend has been attributed to tidal interactions between the star and planet. A constraint on the dissipation parameter Q_*_' follows from the assumption that tides have managed to spin up the star to the observed rate within the age of the system. This technique was applied previously to HATS-18 and WASP-19. Here, we analyze the sample of all 188 known HJs with an orbital period &lt;3.5 days and a "cool" host star (T_eff_&lt;6100 K). We find evidence that the tidal dissipation parameter (Q_*_') increases sharply with forcing frequency, from 10^5^ at 0.5 day^-1^ to 10^7^ at 2 day^-1^. This helps to resolve a number of apparent discrepancies between studies of tidal dissipation in binary stars, HJs, and warm Jupiters. It may also allow for a HJ to damp the obliquity of its host star prior to being destroyed by tidal decay.</description><source format="bibcode">2018AJ....155..165P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/165</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/ApJ/707/446">J/ApJ/707/446 : HAT-P-13 photometry follow-up (Bakos+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/531/A24">J/A+A/531/A24 : WASP-23 photometric and radial velocity data (Triaud+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A88">J/A+A/533/A88 : WASP-50b photometry and radial velocities (Gillon+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/734/109">J/ApJ/734/109 : Follow-up photometry of HAT-P-27 (Beky+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/84">J/ApJ/750/84 : Follow-up photometry and velocity of Qatar 2 (Bryan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/18">J/ApJ/757/18 : Radial velocities for 16 hot Jupiter host stars</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A86">J/A+A/558/A86 : HAT-P-42b and HAT-P-43b ri light curves (Boisse+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A36">J/A+A/559/A36 : Exoplanets WASP-65b and WASP-75b (Gomez Maqueo Chew+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A64">J/A+A/570/A64 : WASP-104b and WASP-106b photometry (Smith+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/148/29">J/AJ/148/29 : Spectroscopy and differential photometry of HATS-4</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/440/1982">J/MNRAS/440/1982 : WASP 95-101 transits (Hellier+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/33">J/AJ/150/33 : Photometry and spectroscopy of HATS-9 and HATS-10</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/150/168">J/AJ/150/168 : Spectroscopy and photometry for HAT-P-50--HAT-P-53</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/586/A93">J/A+A/586/A93 : WASP41 and WASP47 photometric and RV data</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/138">J/AJ/151/138 : Discovery of 2 hot Jupiters KELT-14b + KELT-15b</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/108">J/AJ/152/108 : i filter photometry for HATS-25 through HATS-30</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/127">J/AJ/152/127 : Sloan i follow-up light curves of HATS-18 (Penev+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/152/182">J/AJ/152/182 : iz follow-up photometry of HAT-P-65 and HAT-P-66</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/155/165</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/165</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/165</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/165</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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