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...
Sábháilte in:
| Príomhchruthaitheoirí: | , , , |
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| Formáid: | Artigo |
| Teanga: | Inglês |
| Foilsithe / Cruthaithe: |
IOP Publishing
2026-01-01
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| Sraith: | The Astrophysical Journal |
| Ábhair: | |
| Rochtain ar líne: | https://doi.org/10.3847/1538-4357/ae7f20 |
| Clibeanna: |
Níl clibeanna ann, Bí ar an gcéad duine le clib a chur leis an taifead seo!
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