Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot
Lennart van Sluijs(University of Oxford), David Charbonneau(Harvard University Press), Matteo Brogi(University of Lisbon), Ian J. M. Crossfield(Massachusetts Institute of Technology), Jayne Birkby(University of Amsterdam), Joshua D. Lothringer(University of Arizona), Vivien Parmentier(Centre National de la Recherche Scientifique), Craig Kulesa(University of Arizona), D. W. McCarthy(University of Arizona), Elspeth K. H. Lee(University of Bern)
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