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Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot (2023)

First Author: Van Sluijs L

Attributed to: Warwick Astronomy and Astrophysics Consolidated Grant 2020-2023 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad1103

Publication URI: http://dx.doi.org/10.1093/mnras/stad1103

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2