Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot (2022)
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/10.48550/arxiv.2203.13234
Publication URI: https://arxiv.org/abs/2203.13234
Type: Other