QR kód

The Orbit of Warm Jupiter WASP-106 b is Aligned with its Star

Understanding orbital obliquities, or the misalignment angles between a star’s rotation axis and the orbital axis of its planets, is crucial for unraveling the mechanisms of planetary formation and migration. In this study, we present an analysis of Rossiter–McLaughlin (RM) observations of the warm...

Celý popis

Uloženo v:
Hlavní autoři: Jan-Vincent Harre, Alexis M. S. Smith, Teruyuki Hirano, Szilárd Csizmadia, Amaury H. M. J. Triaud, David R. Anderson
Médium: Artigo
Jazyk:Inglês
Vydáno: IOP Publishing 2023-01-01
Edice:The Astronomical Journal
Témata:
Exoplanet evolution
Exoplanet migration
Radial velocity
Photometry
Transits
On-line přístup:https://doi.org/10.3847/1538-3881/acf46d
Tagy: Přidat tag
Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!

Podobné jednotky