Scaled three-dimensional simulations of giant-planet accretion and disk clearing
astro-ph.EP, astro-ph.SR
Submitted: 2026-10-11
Updated: 2026-10-11
Sources
- Simultaneous gas accretion onto a pair of giant planets: Impact on their final mass and on the protoplanetary disk structure
- Orbital Advection by Interpolation: A Fast and Accurate Numerical Scheme for Super-Fast MHD Flows
- 3D Global Simulations of Accretion onto Gap-opening Planets: Implications for Circumplanetary Disc Structures and Accretion Rates
- Concurrent Accretion and Migration of Giant Planets in their Natal Disks with Consistent Accretion Torque
- FARGO: a fast eulerian transport algorithm for differentially rotating disks
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- Gravitational Microlensing
- Two-stage disruption of resonant chains
- Detectability of resolved hydrogen lines from the accretion shock at gas giants and their CPDs
- Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
- Atmospheric escape fractionates secondary but not primary atmospheres