Turbulence in accretion disks: vorticity generation and angular momentum transport via the global baroclinic instability
HH Klahr, P Bodenheimer - The Astrophysical Journal, 2003 - iopscience.iop.org
In this paper we present the global baroclinic instability as a source for vigorous turbulence
leading to angular momentum transport in Keplerian accretion disks. We show by analytical …
leading to angular momentum transport in Keplerian accretion disks. We show by analytical …
Structured distributions of gas and solids in protoplanetary disks
J Bae, A Isella, Z Zhu, R Martin, S Okuzumi… - ar** by vortices in transitional disks: evidence for non-ideal magnetohydrodynamic effects in protoplanetary disks
Z Zhu, JM Stone - The Astrophysical Journal, 2014 - iopscience.iop.org
We study particle trap** at the edge of a gap opened by a planet in a protoplanetary disk.
In particular, we explore the effects of turbulence driven by the magnetorotational instability …
In particular, we explore the effects of turbulence driven by the magnetorotational instability …
Pebble trap** in vortices: three-dimensional simulations
Disk vortices have been heralded as promising routes for planet formation due to their ability
to trap significant amounts of pebbles. While the gas motions and trap** properties of two …
to trap significant amounts of pebbles. While the gas motions and trap** properties of two …
Analysis of the arm-like structure in the outer disk of PDS 70-Spiral density wave or vortex?
Context. Observing dynamical interactions between planets and disks is key to
understanding their formation and evolution. Two protoplanets have recently been …
understanding their formation and evolution. Two protoplanets have recently been …