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...
Tallennettuna:
| Päätekijät: | , , , , |
|---|---|
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
IOP Publishing
2024-01-01
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| Sarja: | The Astronomical Journal |
| Aiheet: | |
| Linkit: | https://doi.org/10.3847/1538-3881/ad1ab9 |
| Tagit: |
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