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Advection of Potential Temperature in the Atmosphere of Irradiated Exoplanets: A Robust Mechanism to Explain Radius Inflation (2017)

First Author: Tremblin P

Attributed to: Supercomputer support for the Astrophysics Group at the University of Exeter funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aa6e57

Publication URI: http://dx.doi.org/10.3847/1538-4357/aa6e57

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1