[HTML][HTML] Horseshoes and spiral waves: capturing the 3D flow induced by a low-mass planet analytically
JJ Brown, GI Ogilvie - Monthly Notices of the Royal Astronomical …, 2024 - academic.oup.com
The key difficulty faced by 2D models for planet–disc interaction is in appropriately
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
Horseshoes and spiral waves: capturing the 3D flow induced by a low-mass planet analytically
J Brown, G Ogilvie - 2024 - repository.cam.ac.uk
The key difficulty faced by 2D models for planet-disc interaction is in appropriately
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
Horseshoes and spiral waves: capturing the 3D flow induced by a low-mass planet analytically
JJ Brown, GI Ogilvie - Monthly Notices of the Royal Astronomical …, 2024 - academic.oup.com
The key difficulty faced by 2D models for planet–disc interaction is in appropriately
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
Horseshoes and spiral waves: capturing the 3D flow induced by a low-mass planet analytically
JJ Brown, GI Ogilvie - arXiv preprint arXiv:2409.02687, 2024 - arxiv.org
The key difficulty faced by 2D models for planet-disc interaction is in appropriately
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …
accounting for the impact of the disc's vertical structure on the dynamics. 3D effects are often …