Doppler tomography of transiting exoplanets: A prograde, low-inclined orbit for the hot Jupiter CoRoT-11b

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Gandolfi, D ^a   Collier Cameron, A ^b   Endl, M ^c   Lanza, A F ^d   Damiani, C ^d,e   Alonso, R ^f,g   Cochran, W D ^c   Deleuil, M ^e   Fridlund, M ^a   Hatzes, A P ^h   Guenther, E W ^h  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c University of Texas at Austin   (United States)

^d INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^e CNRS   (France)

^f INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^g UNIVERSIDAD DE LA LAGUNA   (Spain)

^h Thüringer Landessternwarte ^*  (Germany)

Author keywords

Binaries: eclipsing; Planet disk interactions; Planet star interactions; Planetary systems; Stars: individual: CoRoT 11

Indexed keywords

SEDIMENTATION; TIME SERIES ANALYSIS; TOMOGRAPHY; UNCERTAINTY ANALYSIS;

ABSOLUTE VALUES; BINARIES:ECLIPSING; DOPPLER; DOPPLER TOMOGRAPHY; EFFECTIVE TEMPERATURE; EXO-PLANETS; HIGH-RESOLUTION SPECTRA; HOST-STARS; JUPITERS; MARKOV CHAIN MONTE CARLO; MASSIVE STARS; PHYSICAL PARAMETERS; PLANETARY SYSTEM; QUALITY FACTORS; SIMULTANEOUS FITTING; SPECTROSCOPIC DATA; SPIN ORBITS; STARS: INDIVIDUAL; STELLAR ROTATION; TIDAL EVOLUTION;

STARS;

EID: 84863219740     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219533     Document Type: Article

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