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J. J. Zanazzi et al 2024 ApJL 967 L29
If the orbits of hot Jupiters can couple to a stellar gravity mode through resonance locking, it may explain the mystery of why the obliquity of these extreme exoplanets correlates with stellar temperature.

Na’ama Hallakoun et al 2024 ApJL 970 L11

White dwarfs in binary systems with a main-sequence companion separated by roughly 1 au are less likely to be massive than single white dwarfs in the field, which may be due to a lack of mergers in this population.
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