collaborators

13 papers

astro-ph.EP2026

Atmospheric Escape Rates of Planets in Stellar Tidal Fields from 3-D Hydrodynamic Simulations

Ritika Sethi, Morgan MacLeod, Sarah Millholland

Thermally driven atmospheric escape, including photo-evaporation and core-powered mass-loss, plays a key role in shaping the evolution of close-in exoplanets, yet most current mode…

astro-ph.EP2026

The Architecture of the 14 Herculis System Suggests Primordial Ejection of a Massive Planet

Tiger Lu, Sarah C. Millholland, Malena Rice +6

The 14 Herculis system hosts two super-Jupiters on eccentric, significantly misaligned orbits. This orbital architecture represents a dynamical puzzle that demands explanation. In…

astro-ph.EP2026

Uncovering the Rapidly Evolving Orbits of the Dynamic TOI-201 System

Ismael Mireles, Solène Ulmer-Moll, Donald Liveoak +47

Studying planetary interactions in exoplanet systems informs theories of planet formation and evolution, providing essential context for understanding our own solar system. We comb…

astro-ph.EP2026

Direct Imaging Constraints on Binary Planets and Exomoons around Epsilon Indi A b

Matson Garza, Mary Anne Limbach, Rachel Bowens-Rubin +6

Epsilon Indi A b is a directly imaged exoplanet orbiting a nearby (3.6 pc) K-dwarf at AU. We analyze archival JWST/MIRI 15 m coronagraphic imaging…

astro-ph.EP2026

Self-consistent Dynamical and Chaotic Tides in the REBOUNDx framework

Donald J. Liveoak, Sarah C. Millholland, Michelle Vick +1

At high eccentricities, tidal forcing excites vibrational modes within orbiting bodies known as dynamical tides. In this paper, we implement the coupled evolution of these modes wi…

astro-ph.EP2025

Exploring Exoplanet Dynamics with JWST: Tides, Rotation, Rings, and Moons

Sarah C. Millholland, Joshua N. Winn

Although nearly 6,000 exoplanets are currently known, in most cases our knowledge is limited to a handful of the planet's orbital characteristics and bulk properties such as radius…