Understanding the atmospheric properties and chemical composition of the ultra-hot Jupiter HAT-P-7b I. Cloud and chemistry mapping (2019)
Attributed to:
Inverse Modelling Methods for the Characterisation of Exoplanetary Atmospheres
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201935771
Publication URI: http://dx.doi.org/10.1051/0004-6361/201935771
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics
ISSN: 0004-6361