Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot

Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spotDOI: info:10.1093/mnras/stad1103v. 5222145–2170
van Sluijs, Lennart, Birkby, Jayne L., Lothringer, Joshua, Lee, Elspeth K. H., Crossfield, Ian J. M., Parmentier, Vivien, Brogi, Matteo, Kulesa, Craig, McCarthy, Don, and Charbonneau, David. 2023. "Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot." Monthly Notices of the Royal Astronomical Society, 522 2145–2170. https://doi.org/10.1093/mnras/stad1103.
ID: 171177
Type: article
Keywords: sao