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astro-ph.EP2026

Flyby-induced high-eccentricity migration and the prevalence of hot Jupiters in M67

Mika V. Kontiainen, Cathie J. Clarke, Andrew J. Winter

Few planetary systems form in isolation. Rather, interactions in their birth environments may sculpt their architectures or drive them into unstable configurations. Here we study t…

astro-ph.EP2025

Hot Jupiter formation in dense stellar clusters: A Monte Carlo model applied to 47 Tucanae

J. A. Wirth, C. J. Clarke, A. J. Winter

We study the efficiency of high-e migration as a pathway for Hot Jupiter formation in the dense globular cluster 47 Tuc. Gravitational N-body simulations are performed to investiga…

astro-ph.EP2025

On Hot Jupiters and Stellar Clustering: The Role of Host Star Demographics

Mika V. Kontiainen, Cathie J. Clarke, Andrew J. Winter

The variation in hot Jupiter (HJ) occurrence across stellar environments holds clues as to the dominant formation channels of these extreme planets. Recent studies suggest HJ hosts…

astro-ph.EP2025

Disc-planet misalignment from an unstable triple system: IRAS04125

Rebecca Nealon, Jeremy L. Smallwood, Hossam Aly +5

The IRAS01425+2902 wide binary system was recently reported to have both a young planet and a puzzling geometric arrangement, where the planet and binary both orbit edge-on, but mi…

astro-ph.EP2025

XUE. Thermochemical Modeling Suggests a Compact and Gas-Depleted Structure for a Distant, Irradiated Protoplanetary Disk

Bayron Portilla-Revelo, Konstantin V. Getman, María Claudia Ramírez-Tannus +14

Unveiling the physical structure of protoplanetary disk is crucial for interpreting the diversity of the exoplanet population. Until recently, the census of the physical properties…