3 papers
astro-ph.EP2025
Exploring Warm Jupiter Migration Pathways with Eccentricities II. Correlations with Host Star Properties and Orbital Separation
Marvin Morgan, Brendan P. Bowler, Quang H. Tran
Warm Jupiters with orbital periods of 10-365 d represent a population of giant planets located well within the water ice line but beyond the region of tidal influence of t…
astro-ph.EP2025
Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters
Marvin Morgan, Brendan P. Bowler, Quang H. Tran +4
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 t…
astro-ph.EP2025
One-third of Sun-like stars are born with misaligned planet-forming disks
Lauren I. Biddle, Brendan P. Bowler, Marvin Morgan +2
Exoplanets are organized in a broad array of orbital configurations that reflect their formation along with billions of years of dynamical processing through gravitational interact…