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...
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| Hlavní autoři: | , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2023-01-01
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| Edice: | The Astrophysical Journal Letters |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/2041-8213/acd552 |
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