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The Period Distribution of Hot Jupiters Is Not Dependent on Host Star Metallicity

The probability that a Sun-like star has a close-orbiting giant planet (period ≲1 yr) increases with stellar metallicity. Previous work provided evidence that the period distribution of close-orbiting giant planets is also linked to metallicity, hinting that there two formation/evolution pathways fo...

Ausführliche Beschreibung

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Bibliografische Detailangaben
Hauptverfasser: Samuel W. Yee, Joshua N. Winn
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2023-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Online-Zugang:https://doi.org/10.3847/2041-8213/acd552
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