Работы, на которые ссылается эта работа

Работ: 81

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

1. SECULAR CHAOS AND THE PRODUCTION OF HOT JUPITERS

   Yanqin Wu, Yoram Lithwick

   Статья2011Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797824

2. Planet formation in discs with inclined binary companions: can primordial spin–orbit misalignment be produced?

   J. J. Zanazzi, Dong Lai

   Статья2018Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797825

3. Damping Obliquities of Hot Jupiter Hosts by Resonance Locking

   J. J. Zanazzi, Janosz W. Dewberry, Eugene Chiang

   Статья2024Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797826

4. Author Correction: Measured spin–orbit alignment of ultra-short-period super-Earth 55 Cancri e

   Lily Zhao, Vedad Kunovac, John M. Brewer +8

   Статья2023Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797828

5. THE OCCURRENCE OF WIDE-ORBIT PLANETS IN BINARY STAR SYSTEMS

   B. Zuckerman

   Статья2014Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797829

6. ANCIENT PLANETARY SYSTEMS ARE ORBITING A LARGE FRACTION OF WHITE DWARF STARS

   B. Zuckerman, C. Melis, B. Klein +2

   Статья2010Цитирований: 1

   ABIABI:AkademIndex/openalex/2026.other.797830