The Orbital Eccentricities of Planets in the Kinematic Thin and Thick Galactic Disks

The orbital eccentricity distribution of exoplanets is shaped by a combination of dynamical processes, reflecting both formation conditions and long-term evolution. Probing the orbital dynamics of planets in the kinematic thin and thick Galactic disks provides insight into the degree to which stella...

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Autors principals:	Sheila Sagear, Sarah Ballard, Kathryne J. Daniel, Adrian M. Price-Whelan, Sóley Ó. Hyman, Gregory J. Gilbert, Christopher Lam
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astronomical Journal
Matèries:	Eccentricity Exoplanet dynamics Exoplanets Milky Way disk Milky Way dynamics
Accés en línia:	https://doi.org/10.3847/1538-3881/ae71bf
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