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dc.creatorCsizmadia, S.en_US
dc.creatorMoutou, C.en_US
dc.creatorDeleuil, M.en_US
dc.creatorCabrera, J.en_US
dc.creatorFridlund, M.en_US
dc.creatorGandolfi, D.en_US
dc.creatorAigrain, S.en_US
dc.creatorAlonso, R.en_US
dc.creatorAlmenara, J. M.en_US
dc.creatorAuvergne, M.en_US
dc.creatorBaglin, A.en_US
dc.creatorBarge, P.en_US
dc.creatorBonomo, A. S.en_US
dc.creatorBorde, P.en_US
dc.creatorBouchy, F.en_US
dc.creatorBruntt, H.en_US
dc.creatorCarone, L.en_US
dc.creatorCarpano, S.en_US
dc.creatorCavarroc, C.en_US
dc.creatorCochran, W.en_US
dc.creatorDeeg, H. J.en_US
dc.creatorDiaz, R. F.en_US
dc.creatorDvorak, R.en_US
dc.creatorEndl, M.en_US
dc.creatorErikson, A.en_US
dc.creatorFerraz-Mello, S.en_US
dc.creatorFruth, T.en_US
dc.creatorGazzano, J. C.en_US
dc.creatorGillon, M.en_US
dc.creatorGuenther, E. W.en_US
dc.creatorGuillot, T.en_US
dc.creatorHatzes, A.en_US
dc.creatorHavel, M.en_US
dc.creatorHebrard, G.en_US
dc.creatorJehin, E.en_US
dc.creatorJorda, L.en_US
dc.creatorLeger, A.en_US
dc.creatorLlebaria, A.en_US
dc.creatorLammer, H.en_US
dc.creatorLovis, C.en_US
dc.creatorMacQueen, P. J.en_US
dc.creatorMazeh, T.en_US
dc.creatorOllivier, M.en_US
dc.creatorPatzold, M.en_US
dc.creatorQueloz, D.en_US
dc.creatorRauer, H.en_US
dc.creatorRouan, D.en_US
dc.creatorSanterne, A.en_US
dc.creatorSchneider, J.en_US
dc.creatorTingley, B.en_US
dc.creatorTitz-Weider, R.en_US
dc.creatorWuchterl, G.en_US
dc.date.accessioned2016-04-22T19:46:54Z
dc.date.available2016-04-22T19:46:54Z
dc.date.issued2011-07en
dc.identifierdoi:10.15781/T2KB8T
dc.identifier.citationCsizmadia, Sz, C. Moutou, M. Deleuil, J. Cabrera, M. Fridlund, D. Gandolfi, S. Aigrain et al. >Transiting exoplanets from the CoRoT space mission-XVII. The hot Jupiter CoRoT-17b: a very old planet.> Astronomy & Astrophysics, Vol. 531 (Jul., 2011): A41.en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://hdl.handle.net/2152/34466
dc.description.abstractWe report on the discovery of a hot Jupiter-type exoplanet, CoRoT-17b, detected by the CoRoT satellite. It has a mass of 2.43 +/- 0.30 M-Jup and a radius of 1.02 +/- 0.07 R-Jup, while its mean density is 2.82 +/- 0.38 g/cm(3). CoRoT-17b is in a circular orbit with a period of 3.7681 +/- 0.0003 days. The host star is an old (10.7 +/- 1.0 Gyr) main-sequence star, which makes it an intriguing object for planetary evolution studies. The planet's internal composition is not well constrained and can range from pure H/He to one that can contain similar to 380 earth masses of heavier elements.en_US
dc.description.sponsorshipW.M. Keck Foundationen_US
dc.description.sponsorshipSpanish Ministerio de Ciencia e Innovacion ESP2007-65480-C02-02en_US
dc.description.sponsorshipNational Aeronautics and Space Administration NNX09AB30Gen_US
dc.description.sponsorshipNational Science Foundationen_US
dc.description.sponsorshipFond National de la Recherche Scientifique, FNRS FRFC 2.5.594.09.Fen_US
dc.description.sponsorshipDLR 50 OW 204, 50 OW 0603, 50QP07011en_US
dc.language.isoEnglishen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.subjecttechniques: photometricen_US
dc.subjecttechniques: radial velocitiesen_US
dc.subjecttechniques:en_US
dc.subjectspectroscopicen_US
dc.subjectplanetary systemsen_US
dc.subjectabundance analysisen_US
dc.subjectstarsen_US
dc.subjectdwarfen_US
dc.subjectmetallicityen_US
dc.subjectisochronesen_US
dc.subjectevolutionen_US
dc.subjectspectraen_US
dc.subjectsearchen_US
dc.subjectmodelsen_US
dc.subjectsolaren_US
dc.subjectastronomy & astrophysicsen_US
dc.titleTransiting Exoplanets From The CoRoT Space Mission XVII. The Hot Jupiter CoRoT-17B: A Very Old Planeten_US
dc.typeArticleen_US
dc.description.departmentMcDonald Observatoryen_US
dc.identifier.doi10.1051/0004-6361/201117009en_US
dc.contributor.utaustinauthorCochran, W. D.en_US
dc.contributor.utaustinauthorEndl, M.en_US
dc.contributor.utaustinauthorMacQueen, P.J.en_US
dc.relation.ispartofserialAstronomy & Astrophysicsen_US


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