Substructures induced by dust drag in protoplanetary disks
Dust substructures observed in protoplanetary disks are commonly attributed to embedded planets; however, intrinsic gas-dust interactions can also generate complex morphologies. We performed two-dimensional, axisymmetric simulations of gas and dust that include dust back-reaction and parameterized t...
Gorde:
| Egile Nagusiak: | , , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
EDP Sciences
2026-06-01
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| Saila: | Astronomy & Astrophysics |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.aanda.org/articles/aa/full_html/2026/06/aa59809-26/aa59809-26.html |
| Etiketak: |
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