Evidence for Nightside Water Emission Found in Transit of Ultra-hot Jupiter WASP-33 b
To date, the dayside thermal structure of ultra-hot Jupiters (UHJs) is generally considered to be inverted, but their nightside thermal structure has been less explored. Here, we explore the impact of nightside thermal emission on high-resolution infrared transmission spectroscopy, which should not...
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| Автори: | , , , , |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2024-01-01
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| Серія: | The Astrophysical Journal Letters |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/2041-8213/ad65cf |
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