Orbital Alignment of the Eccentric Warm Jupiter TOI-677 b

Orbital Alignment of the Eccentric Warm Jupiter TOI-677 b

Warm Jupiters lay out an excellent laboratory for testing models of planet formation and migration. Their separation from the host star makes tidal reprocessing of their orbits ineffective, which preserves the orbital architectures that result from the planet-forming process. Among the measurable pr...

Full description

Bibliographic Details
Main Authors: Elyar Sedaghati, Andrés Jordán, Rafael Brahm, Diego J. Muñoz, Cristobal Petrovich, Melissa J. Hobson
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Exoplanets
Planetary alignment
Exoplanet dynamics
Exoplanet migration
Radial velocity
Transits
Online Access:https://doi.org/10.3847/1538-3881/acea84

Internet

https://doi.org/10.3847/1538-3881/acea84

Similar Items