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Иш: Origins of Hot Jupiters from the Stellar Obliquity Distribution

1. TOI-1259Ab: A warm Jupiter orbiting a K-dwarf white-dwarf binary on a low-obliquity orbit

   Hugo Veldhuis, Juan I. Espinoza-Retamal, Guðmundur Stefánsson +25

   МақолаStellar, planetary, and galactic studiesAstronomy and Astrophysics20260 иқтибос

   ABIABI:AkademIndex/openalex/2026.article.000475