Coupled Thermal–Chemical Evolution Models of Sub-Neptunes Reveal Atmospheric Signatures of Their Formation Location
The observed masses and radii of sub-Neptunes are typically explained by the gas dwarf or water world scenarios. While their evolutionary history on a population level has been proposed as a method to distinguish between these compositions, previous evolutionary models neglected the crucial role of...
Gardado en:
| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
IOP Publishing
2026-01-01
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| Series: | The Astrophysical Journal |
| Assuntos: | |
| Acceso en liña: | https://doi.org/10.3847/1538-4357/ae4c47 |
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