12 citations · 16 across the 2 of their papers we have counts for
2 papers
astro-ph.EP2024★ 4 cited
The coevolution of migrating planets and their pulsating stars through episodic resonance locking
Jared Bryan, Julien de Wit, Meng Sun +2
Hot Jupiters are expected to form far from their host star and move toward close-in, circular orbits via a smooth, monotonic decay due to mild and constant tidal dissipation. Yet,…
astro-ph.EP2023★ 12 cited
Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 c
Zoë L. de Beurs, Julien de Wit, Alexander Venner +5
One possible formation mechanism for Hot Jupiters is that high-eccentricity gas giants experience tidal interactions with their host star that cause them to lose orbital energy and…