Transiting Exoplanets From The Corot Space Mission XIV. CoRoT-11B: A Transiting Massive >Hot-Jupiter> In A Prograde Orbit Around A Rapidly Rotating F-Type Star

dc.contributor.utaustinauthorCochran, W. D.en_US
dc.contributor.utaustinauthorEndl, M.en_US
dc.contributor.utaustinauthorMacQueen, P.J.en_US
dc.creatorGandolfi, D.en_US
dc.creatorHebrard, G.en_US
dc.creatorAlonso, R.en_US
dc.creatorDeleuil, M.en_US
dc.creatorGuenther, E. W.en_US
dc.creatorFridlund, M.en_US
dc.creatorEndl, M.en_US
dc.creatorEigmuller, P.en_US
dc.creatorCsizmadia, S.en_US
dc.creatorHavel, M.en_US
dc.creatorAigrain, S.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.creatorCabrera, J.en_US
dc.creatorCarpano, S.en_US
dc.creatorCarone, L.en_US
dc.creatorCochran, W. D.en_US
dc.creatorDeeg, H. J.en_US
dc.creatorDvorak, R.en_US
dc.creatorEisloffel, J.en_US
dc.creatorErikson, A.en_US
dc.creatorFerraz-Mello, S.en_US
dc.creatorGazzano, J. C.en_US
dc.creatorGibson, N. B.en_US
dc.creatorGillon, M.en_US
dc.creatorGondoin, P.en_US
dc.creatorGuillot, T.en_US
dc.creatorHartmann, M.en_US
dc.creatorHatzes, A.en_US
dc.creatorJorda, L.en_US
dc.creatorKabath, P.en_US
dc.creatorLeger, A.en_US
dc.creatorLlebaria, A.en_US
dc.creatorLammer, H.en_US
dc.creatorMacQueen, P. J.en_US
dc.creatorMayor, M.en_US
dc.creatorMazeh, T.en_US
dc.creatorMoutou, C.en_US
dc.creatorOllivier, M.en_US
dc.creatorPatzold, M.en_US
dc.creatorPepe, F.en_US
dc.creatorQueloz, D.en_US
dc.creatorRauer, H.en_US
dc.creatorRouan, D.en_US
dc.creatorSamuel, B.en_US
dc.creatorSchneider, J.en_US
dc.creatorStecklum, B.en_US
dc.creatorTingley, B.en_US
dc.creatorUdry, S.en_US
dc.creatorWuchterl, G.en_US
dc.date.accessioned2016-04-22T19:46:52Z
dc.date.available2016-04-22T19:46:52Z
dc.date.issued2010-12en
dc.description.abstractThe CoRoT exoplanet science team announces the discovery of CoRoT-11b, a fairly massive hot-Jupiter transiting a V = 12.9 mag F6 dwarf star (M(*) = 1.27 +/- 0.05 M(circle dot), R(*) = 1.37 +/- 0.03 R(circle dot), T(eff) = 6440 +/- 120 K), with an orbital period of P = 2.994329 +/- 0.000011 days and semi-major axis a = 0.0436 +/- 0.005 AU. The detection of part of the radial velocity anomaly caused by the Rossiter-McLaughlin effect shows that the transit-like events detected by CoRoT are caused by a planet-sized transiting object in a prograde orbit. The relatively high projected rotational velocity of the star (upsilon sin i(star) = 40 +/- 5 km s(-1)) places CoRoT-11 among the most rapidly rotating planet host stars discovered so far. With a planetary mass of M(p) = 2.33 +/- 0.34 M(Jup) and radius R(p) = 1.43 +/- 0.03 R(Jup), the resulting mean density of CoRoT-11b (rho(p) = 0.99 +/- 0.15 g/cm(3)) can be explained with a model for an inflated hydrogen-planet with a solar composition and a high level of energy dissipation in its interior.en_US
dc.description.departmentMcDonald Observatoryen_US
dc.description.sponsorshipW.M. Keck Foundationen_US
dc.description.sponsorshipSpanish Ministerio de Ciencia e Innovacion ESP2007-65480-C02-02en_US
dc.description.sponsorshipDLR 50OW0204, 50OW0603, 50QP07011en_US
dc.identifierdoi:10.15781/T2TV38
dc.identifier.citationGandolfi, D., G. Hébrard, R. Alonso, M. Deleuil, E. W. Guenther, M. Fridlund, M. Endl et al. >Transiting exoplanets from the CoRoT space mission-XIV. CoRoT-11b: a transiting massive “hot-Jupiter” in a prograde orbit around a rapidly rotating F-type star.> Astronomy & Astrophysics, Vol. 524 (Dec., 2010): A55.en_US
dc.identifier.doi10.1051/0004-6361/201015132en_US
dc.identifier.issn0004-6361en_US
dc.identifier.urihttp://hdl.handle.net/2152/34464
dc.language.isoEnglishen_US
dc.relation.ispartofserialAstronomy & Astrophysicsen_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.subjectplanetary systemsen_US
dc.subjecttechniques: photometricen_US
dc.subjecttechniques: radialen_US
dc.subjectvelocitiesen_US
dc.subjecttechniques: spectroscopicen_US
dc.subjectgas-giant planeten_US
dc.subjectechelle spectrometeren_US
dc.subjectphotometric-methoden_US
dc.subjectabundanceen_US
dc.subjectanalysisen_US
dc.subjectsearch-programsen_US
dc.subjectg-dwarfen_US
dc.subjectlithiumen_US
dc.subjectstellaren_US
dc.subjectparametersen_US
dc.subjectsystemsen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleTransiting Exoplanets From The Corot Space Mission XIV. CoRoT-11B: A Transiting Massive >Hot-Jupiter> In A Prograde Orbit Around A Rapidly Rotating F-Type Staren_US
dc.typeArticleen_US

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