Journal article
Connecting planet formation and astrochemistry
Abstract
The chemical composition of planetary atmospheres has long been thought to store information regarding where and when a planet accretes its material. Predicting this chemical composition theoretically is a crucial step in linking observational studies to the underlying physics that govern planet formation. As a follow-up to an earlier study of ours on hot Jupiters, we present a population of warm Jupiters (semi-major axis between 0.5 and 4 AU) …
Authors
Cridland AJ; van Dishoeck EF; Alessi M; Pudritz RE
Journal
Astronomy & Astrophysics, Vol. 642, ,
Publisher
EDP Sciences
Publication Date
10 2020
DOI
10.1051/0004-6361/202038767
ISSN
0004-6361