Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters

Giant planets are expected to predominantly form beyond the water-ice line and occasionally undergo inward migration. Unlike hot Jupiters, which can result from high-eccentricity tidal migration, warm Jupiters between 0.1 and 1 au (≈10–365 days) are in many ways more challenging to explain because t...

Disgrifiad llawn

Manylion Llyfryddiaeth

Prif Awduron:	Marvin Morgan, Brendan P. Bowler, Quang H. Tran, Robert A. Wittenmyer, Duncan J. Wright, George Zhou, Tyler R. Fairnington
Fformat:	Artigo
Iaith:	Inglês
Cyhoeddwyd:	IOP Publishing 2025-01-01
Cyfres:	The Astrophysical Journal Supplement Series
Pynciau:	Exoplanet migration Exoplanet evolution
Mynediad Ar-lein:	https://doi.org/10.3847/1538-4365/adf55d
Tagiau:	Ychwanegu Tag Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!