Why is it So Hot in Here? Exploring Population Trends in Spitzer Thermal Emission Observations of Hot Jupiters Using Planet-specific, Self-consistent Atmospheric Models (2021)
Attributed to:
A comprehensive study of stars, disks and exoplanets
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ac27b2
Publication URI: http://dx.doi.org/10.3847/1538-4357/ac27b2
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2