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<ri:Resource created="2016-10-10T14:00:04Z" 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>Stars with M_p_sin(i)&gt;0.1M_Jup_ hot Jupiter</title><shortName>J/ApJ/825/62</shortName><identifier>ivo://CDS.VizieR/J/ApJ/825/62</identifier><altIdentifier>doi:10.26093/cds/vizier.18250062</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Schlaufman K.C.</name></creator><creator><name>Winn J.N.</name></creator><date role="Updated">2023-02-13T15:23:09Z</date><date role="Created">2016-10-10T14:00:04Z</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>solar-system-planets</subject><description>The origin of Jupiter-mass planets with orbital periods of only a few days is still uncertain. It is widely believed that these planets formed near the water-ice line of the protoplanetary disk, and subsequently migrated into much smaller orbits. Most of the proposed migration mechanisms can be classified either as disk-driven migration, or as excitation of a very high eccentricity followed by tidal circularization. In the latter scenario, the giant planet that is destined to become a hot Jupiter spends billions of years on a highly eccentric orbit, with apastron near the water-ice line. Eventually, tidal dissipation at periastron shrinks and circularizes the orbit. If this is correct, then it should be especially rare for hot Jupiters to be accompanied by another giant planet interior to the water-ice line. Using the current sample of giant planets discovered with the Doppler technique, we find that hot Jupiters with P_orb_&lt;10d are no more or less likely to have exterior Jupiter-mass companions than longer-period giant planets with P_orb_&gt;=10d. This result holds for exterior companions both inside and outside of the approximate location of the water-ice line. These results are difficult to reconcile with the high-eccentricity migration scenario for hot Jupiter formation.</description><source format="bibcode">2016ApJ...825...62S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/825/62</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/I/259">I/259 : The Tycho-2 Catalogue (Hog+ 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/821/89">J/ApJ/821/89 : 12yrs of RV obs. of exoplanet systems (Bryan+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A64">J/A+A/587/A64 : Physical properties of giant exoplanets (Santerne+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/123/412">J/PASP/123/412 : Exoplanet Orbit Database (Wright+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/168">J/ApJ/709/168 : Eccentric orbits in exoplanets (Anglada-Escude+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/697/544">J/ApJ/697/544 : Planets orbiting metal-poor dwarfs. II. (Sozzetti+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/693/1084">J/ApJ/693/1084 : Ten new and updated multiplanet systems (Wright+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/496/513">J/A+A/496/513 : RV of 6 stars with long-period giant planets (Moutou+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/479/865">J/A+A/479/865 : CoRoT exoplanet candidates (Loeillet+, 2008)</relatedResource><relatedResource>http://exoplanets.org/ : Exoplanet Orbit Database home page</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/825/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/825/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/825/62</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/825/62</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/825/62</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/825/62</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/825/62/table1 (Exoplanet systems in our Doppler sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/825/62/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/825/62/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/825/62/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.5798972</ra><dec>-49.0751864</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/311 431 679 725 748 1544 1597 2110 2152 2374 2416 2472 2497 3663 3876 3932 4136 4528 4881 5009 5067 5309 5522 5718 6237 6760 6791 6821 6831 7746 8357 8843 9403 9459 9483 9662 9843 10079 11087 11267 11326 11589 11910 12024 12465 12502 12644 12899 12983 13808 14412 14419 14434 14525 14548 14682 15174 16627 16652 16707 16783 16823 17341 17496 17587 17641 17730 17954 18614 18666 18747 18821 18835 19619 19904 19912 20145 20557 20582 20746 21003 21326 21838 21906 22036 22252 22590 22654 22837 23013 23030 23201 23414 23646 23681 24019 24178 24831 25401 25875 25939 26183 26242 26575 26707 26790 26901 26978 26997 27018 27088 27164 27616 27750 27975 28130 28571 28763 28767 28865 29291 29513 29541 30015 30378 30526 30707 31374 31494 31860 31874 32561 32848 32930 33042 33182 33243 33258 33430 33510 33630 33717 33923 33974 34905 34951 35079 35362 35392 35415 35442 35532 35907 35954 36506 36697 37018 37461 37573 37954-37955 38414 38545 38728 38998 39257 39280 39364 39446 39646 39926 40066 40101 40400 40442 40985 41058 41167 41432 41446 41515 41607 41724 42044 42221 42248 42281 42318 42333 42386 42510 42570 42760 42934 43012 43228 43639 43677 43813 43818 43911 44243 44398 44740 45168 45364 45624 45717 45865 46111 46215 46297 46306 46800 46843 46967 47550 47590 47930 48105 48402 48519 48530 48545</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/825/62?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/ApJ/825/62/table1</name><description>Exoplanet systems in our Doppler sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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