Posted in astro-ph.EP · 2026-09-02 · Juan I. Espinoza-Retamal, Joshua N. Winn, Rafael Brahm, Luke B. Handley, Elise Koo, Caleb Lammers, Cristobal Petrovich, Guðmundur Stefánsson, Andrés Jordán, Xian-Yu Wang, Songhu Wang, Nicholas Saunders, Erik A. Petigura, Lauren M. Weiss, Ashley D. Baker, Theron W. Carmichael, Fei Dai, Jerry Edelstein, Jack Foley, Benjamin J. Fulton, Steven Giacalone, Steven R. Gibson, Samuel Halverson, Andrew W. Howard, Howard Isaacson, Emma McIntyre, Pranav H. Premnath, Maleah Rhem, Kodi Rider, Ryan A. Rubenzahl, Arpita Roy, Christopher Smith, Judah Van Zandt, Josh Walawender, Elina Y. Zhang, Jingyi Zhang
Stellar obliquities provide important clues as to the formation and migration histories of planetary systems, but measurements remain scarce for Neptune-mass planets, especially those orbiting hot stars (above the Kraft break). Here we present observations of the Rossiter-McLaughlin effect in the hot-star/hot-Neptune system WASP-195...