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...
Guardado en:
| Autores principales: | , , , , , |
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
IOP Publishing
2023-01-01
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| Colección: | The Astronomical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-3881/acf46d |
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