Gas Giants Formed by Gravitational Instability May Accrete Atmospheres with Superstellar Carbon-to-oxygen Ratios
Characterizing the atmospheric compositions of exoplanets, along with determining properties such as their mass, mean density, and orbital configuration, are thought to be an effective means for differentiating between various formation and evolution scenarios. Exoplanet atmospheric C/O ratios, when...
שמור ב:
| מחבר ראשי: | |
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| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
IOP Publishing
2026-01-01
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| סדרה: | The Astrophysical Journal |
| נושאים: | |
| גישה מקוונת: | https://doi.org/10.3847/1538-4357/ae5ba7 |
| תגים: |
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