A cloudy fit to the atmosphere of WASP-107 b
Context. WASP-107 b has been observed comprehensively by JWST in the near- and mid-IR bands, meaning we can probe its composition and internal dynamics. Recent analyses reveal a 8 − 10 μm silicate feature, but it remains uncertain how silicate clouds form on this planet. Aims. We aim to fit the comp...
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| Autori principali: | , , , , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
EDP Sciences
2026-04-01
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| Serie: | Astronomy & Astrophysics |
| Soggetti: | |
| Accesso online: | https://www.aanda.org/articles/aa/full_html/2026/04/aa58447-25/aa58447-25.html |
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