Detection of titanium oxide in the atmosphere of a hot Jupiter. (2017)
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/10.1038/nature23651
PubMed Identifier: 28905896
Publication URI: http://europepmc.org/abstract/MED/28905896
Type: Journal Article/Review
Volume: 549
Parent Publication: Nature
Issue: 7671
ISSN: 0028-0836