Interior dynamics of envelopes around disk-embedded planets
In the core accretion scenario, forming planets start to acquire gaseous envelopes while accreting solids. Conventional 1D models assume envelopes to be static and isolated. However, recent 3D simulations demonstrate dynamic gas exchange from the envelope to the surrounding disk. This process is con...
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| Asıl Yazarlar: | , |
|---|---|
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
EDP Sciences
2026-03-01
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| Seri Bilgileri: | Astronomy & Astrophysics |
| Konular: | |
| Online Erişim: | https://www.aanda.org/articles/aa/full_html/2026/03/aa57579-25/aa57579-25.html |
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