Next-generation Atmosphere Models for Giant Planets with Application to Coupled Interior Composition and Spectral Evolution. I. Cloudless Models with Equilibrium Chemistry
We present updated atmosphere models designed for calculating the postformation evolution and cooling of giant planets with masses between 0.3 and 10 M _J . Our tables provide the entropy in the convective region at the base of the atmosphere, temperature ( T )–pressure ( P ) profiles, and emergent...
שמור ב:
| Principais autores: | , , , |
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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/ae7f20 |
| תגים: |
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