New Rossiter-McLaughlin measurements show two hot Jupiters around M dwarfs, TOI-3714 b and TOI-5293 A b, have aligned stellar obliquities, and a toy model suggests Kozai-Lidov migration is most efficient around M dwarfs.
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Aligned Stellar Obliquities for Two Hot Jupiter-hosting M Dwarfs Revealed by MAROON-X: Implications for Hot Jupiter Formation
New Rossiter-McLaughlin measurements show two hot Jupiters around M dwarfs, TOI-3714 b and TOI-5293 A b, have aligned stellar obliquities, and a toy model suggests Kozai-Lidov migration is most efficient around M dwarfs.