Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations
Transmission spectroscopy supports the presence of uncharacterized, light-scattering and -absorbing hazes in the atmospheres of many exoplanets. The complexity of factors influencing the formation, 3D transport, radiative impact, and removal of hazes makes it challenging to match theoretical models...
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| Principais autores: | , , , , |
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| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
IOP Publishing
2024-01-01
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| Serier: | The Astronomical Journal |
| Fag: | |
| Online adgang: | https://doi.org/10.3847/1538-3881/ad1ab9 |
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