Sibling sub-Neptunes around sibling M dwarfs: TOI-521 and TOI-912
Context. Sub-Neptunes are absent in the Solar System, yet they are the most common category of planets found in our Galaxy. This kind of planet challenges the internal structure models, prompts investigations into its formation and evolution, and pushes atmospheric characterisation studies to break...
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| Médium: | Artigo |
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EDP Sciences
2026-01-01
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| Edice: | Astronomy & Astrophysics |
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| On-line přístup: | https://www.aanda.org/articles/aa/full_html/2026/01/aa57304-25/aa57304-25.html |
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