Reading between the rings: observed dust ring properties as probes of planet masses
Amena Faruqi, Jessica Speedie, Ralph E. Pudritz, Farzana Meru
astro-ph.EP
Submitted: 2026-05-26
Comments: 20 pages, 12 figures. Accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Leaky Dust Traps in Planet-Embedded Protoplanetary Disks
- Sequential giant planet formation initiated by disc substructure
- Hydro-, Magnetohydro-, and Dust-Gas Dynamics of Protoplanetary Disks
Related papers
- PDS 70 c and SR 12 c: Observational Constraints on Giant-Planet and Satellite Formation
- 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
- The Occurrence Rate of Nearby Planetary Companions to Hot Jupiters