Pseudo-2D Modelling of Heat Redistribution Through H$_2$ Thermal Dissociation/Recombination: Consequences for Ultra-Hot Jupiters (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/10.48550/arxiv.2104.14376
Publication URI: https://arxiv.org/abs/2104.14376
Type: Other