Secular evolution of viscous and self-gravitating protoplanetary discs with magnetic winds

arXiv:2609.17526 · astro-ph.EP · Submitted 2026-09-15 · Read on arXiv

astro-ph.EP

Submitted: 2026-09-15

Updated: 2026-09-15

Comments: Accepted for publication in MNRAS

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 14× in this paper · explained in 2 episodes
• Angular Momentum Transport — 12× in this paper · explained in 3 episodes
• Angular Momentum Loss — 2× in this paper · explained in 1 episode
• Momentum transfer — 2× in this paper · explained in 2 episodes
• Ambipolar Diffusion — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

• Structured Distributions of Gas and Solids in Protoplanetary Disks
• Initial Conditions of Planet Formation: Lifetimes of Primordial Disks
• Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation
• Disc lifetime distribution as a function of the mass of host star
• Nonthermal Velocity Dispersion in the Outer Disk of HL Tau
• Transport and Accretion in Planet-Forming 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