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K2-29 b/WASP-152 b: AN ALIGNED AND INFLATED HOT JUPITER IN A YOUNG VISUAL BINARY

hal.structure.identifierCentro de Astrofísica da Universidade do Porto [CAUP]
dc.contributor.authorSANTERNE, A.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorHÉBRARD, G.
dc.contributor.authorLILLO-BOX, J.
dc.contributor.authorARMSTRONG, D. J.
hal.structure.identifierVirologia
dc.contributor.authorBARROS, S. C. C.
hal.structure.identifierUniversité Paris-Sud - Paris 11 [UP11]
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorDEMANGEON, O.
hal.structure.identifierDepartamento de Astrofisica [Madrid]
hal.structure.identifierCalar Alto Observatory
dc.contributor.authorBARRADO, D.
dc.contributor.authorDEBACKERE, A.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorDELEUIL, M.
dc.contributor.authorDELGADO MENA, E.
dc.contributor.authorMONTALTO, M.
dc.contributor.authorPOLLACCO, D.
dc.contributor.authorOSBORN, H. P.
dc.contributor.authorSOUSA, S. G.
hal.structure.identifierJoseph Louis LAGRANGE [LAGRANGE]
dc.contributor.authorABE, L.
hal.structure.identifierCentro de Astrofísica da Universidade do Porto [CAUP]
dc.contributor.authorADIBEKYAN, V.
hal.structure.identifierInstituto de Astrofisica de Canarias [IAC]
dc.contributor.authorALMENARA, J. -M.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorANDRÉ, P.
dc.contributor.authorARLIC, G.
dc.contributor.authorBARTHE, G.
hal.structure.identifierCOMUE Université Côte d'Azur (2015-2019) [COMUE UCA]
dc.contributor.authorBENDJOYA, P.
hal.structure.identifierGeneva Observatory
hal.structure.identifierCdR & CdL group
dc.contributor.authorBEHREND, R.
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorBOISSE, I.
hal.structure.identifierObservatoire de Haute-Provence [OHP]
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorBOUCHY, F.
dc.contributor.authorBOUSSIER, H.
dc.contributor.authorBRETTON, M.
dc.contributor.authorBROWN, D. J. A.
hal.structure.identifierInstitut de Mécanique Céleste et de Calcul des Ephémérides [IMCCE]
dc.contributor.authorCARRY, B.
dc.contributor.authorCAILLEAU, A.
dc.contributor.authorCONSEIL, E.
dc.contributor.authorCOULON, G.
dc.contributor.authorCOURCOL, B.
dc.contributor.authorDAUCHET, B.
dc.contributor.authorDALOUZY, J. -C.
dc.contributor.authorDELDEM, M.
dc.contributor.authorDESORMIERES, O.
dc.contributor.authorDUBREUIL, P.
dc.contributor.authorFEHRENBACH, J. -M.
dc.contributor.authorFERRATFIAT, S.
dc.contributor.authorGIRELLI, R.
dc.contributor.authorGREGORIO, J.
dc.contributor.authorJAECQUES, S.
hal.structure.identifierObservatoire Chante-Perdrix
dc.contributor.authorKUGEL, F.
hal.structure.identifierSchool of Physics and Astronomy [Cardiff]
dc.contributor.authorKIRK, J.
dc.contributor.authorLABREVOIR, O.
dc.contributor.authorLACHURIE, J. -C.
dc.contributor.authorLAM, K. W. F.
hal.structure.identifierHôpital Européen Georges Pompidou [APHP] [HEGP]
dc.contributor.authorLE GUEN, P.
dc.contributor.authorMARTINEZ, Pedro
dc.contributor.authorMAURIN, L. P. A.
dc.contributor.authorMCCORMAC, J.
dc.contributor.authorPIOPPA, J-B.
dc.contributor.authorQUADRI, U.
dc.contributor.authorRAJPUROHIT, A.
hal.structure.identifierDépartement RadioChimie et Procédés [DRCP]
dc.contributor.authorREY, J.
dc.contributor.authorRIVET, J. -P.
hal.structure.identifierUniversité Laval [Québec] [ULaval]
dc.contributor.authorROY, R.
hal.structure.identifierCentro de Astrofísica da Universidade do Porto [CAUP]
hal.structure.identifierDepartamento de Física e Astronomia [Porto] [DFA/FCUP]
dc.contributor.authorSANTOS, N. C.
dc.contributor.authorSIGNORET, F.
dc.contributor.authorSTRABLA, L.
dc.contributor.authorSUAREZ, O.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorTOUBLANC, D.
dc.contributor.authorTSANTAKI, M.
dc.contributor.authorVIENNEY, J. -M.
dc.contributor.authorWILSON, P. A.
dc.contributor.authorBACHSCHMIDT, M.
hal.structure.identifierInstitut de Mécanique Céleste et de Calcul des Ephémérides [IMCCE]
dc.contributor.authorCOLAS, Florent
dc.contributor.authorGERTEIS, O.
dc.contributor.authorLOUIS, P.
dc.contributor.authorMARIO, J. -C.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorMARLOT, C.
dc.contributor.authorMONTIER, J.
dc.contributor.authorPERROUD, V.
dc.contributor.authorPIC, V.
hal.structure.identifierCourbes de rotation d'astéroïdes, de comètes et d'étoiles variables [CdR & CdL group]
dc.contributor.authorROMEUF, D.
dc.contributor.authorUBAUD, S.
dc.contributor.authorVERILHAC, D.
dc.date.accessioned2024-04-25T08:06:48Z
dc.date.available2024-04-25T08:06:48Z
dc.date.issued2016-06
dc.identifier.issn0004-637X
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/199336
dc.description.abstractEnIn the present paper we report the discovery of a new hot Jupiter, K2-29 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25 days, a mass of 0.73 +/- 0.04M(sic), and a radius of 1.19 +/- 0.02 R(sic). The host star is a relatively bright (V = 12.5) G7 dwarf with a nearby K5V companion. Based on stellar rotation and the abundance of lithium, we find that the system might be as young as similar to 450 Myr. The observation of the Rossiter-McLaughlin effect shows that the planet is aligned with respect to the stellar spin. Given the deep transit (20 mmag), the magnitude of the star and the presence of a nearby stellar companion, the planet is a good target for both space- and ground-based transmission spectroscopy, in particular in the near-infrared where both stars are relatively bright.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.title.enK2-29 b/WASP-152 b: AN ALIGNED AND INFLATED HOT JUPITER IN A YOUNG VISUAL BINARY
dc.typeArticle de revueen_US
dc.identifier.doi10.3847/0004-637X/824/1/55
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1601.07680
bordeaux.journalThe Astrophysical Journalen_US
bordeaux.volume824
bordeaux.hal.laboratoriesEPOC : Environnements et Paléoenvironnements Océaniques et Continentaux - UMR 5805en_US
bordeaux.issue1
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionCNRS
bordeaux.peerReviewedoui
bordeaux.import.sourcehal
hal.identifierhal-01440104
hal.version1
hal.popularnon
hal.audienceInternationale
hal.exportfalse
workflow.import.sourcehal
dc.rights.ccPas de Licence CCen_US
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