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)

First Author: Goyal J
Attributed to:  Research in Astrophysics at The University of Bristol 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