Evidence That the Occurrence Rate of Hot Jupiters around Sun-like Stars Decreases with Stellar Age
We investigate how the occurrence rate of giant planets (minimum mass > 0.3 M _Jup ) around Sun-like stars depends on the age, mass, and metallicity of their host stars. We develop a hierarchical Bayesian framework to infer the number of planets per star (NPPS) as a function of both planetary and st...
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/acff71 |
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