activity
20052022
most citedThree-Dimensional Vortices in Stratified Protoplanetary Disks

149 citations · 679 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2022★ 56 cited

Hydro-, Magnetohydro-, and Dust-Gas Dynamics of Protoplanetary Disks

G. Lesur, B. Ercolano, M. Flock +16

The building of planetary systems is controlled by the gas and dust dynamics of protoplanetary disks. While the gas is simultaneously accreted onto the central star and dissipated…

astro-ph.SR2018★ 36 cited

Zombie Vortex Instability. III. Persistence with Nonuniform Stratification and Radiative Damping

Joseph Barranco, Suyang Pei, Philip Marcus

The Zombie Vortex Instability (ZVI) occurs in the dead zones of protoplanetary disks (PPDs) where perturbations excite baroclinic critical layers, generating "zombie" vortices and…

astro-ph.SR2016★ 36 cited

Zombie Vortex Instability. II. Thresholds to Trigger Instability and the Properties of Zombie Turbulence in the Dead Zones of Protoplanetary Disks

Philip S. Marcus, Suyang Pei, Chung-Hsiang Jiang +1

In Zombie Vortex Instability (ZVI), perturbations excite critical layers in stratified, rotating shear flow (as in protoplanetary disks), causing them to generate vortex layers, wh…

astro-ph.SR2014★ 126 cited

Zombie Vortex Instability I: A Purely Hydrodynamic Instability to Resurrect the Dead Zones of Protoplanetary Disks

Philip Marcus, Suyang Pei, Chung-Hsiang Jiang +3

There is considerable interest in hydrodynamic instabilities in dead zones of protoplanetary disks as a mechanism for driving angular momentum transport and as a source of particle…

astro-ph.EP2010★ 26 cited

Forming Planetesimals by Gravitational Instability: II. How Dust Settles to its Marginally Stable State

Aaron T. Lee, Eugene Chiang, Xylar Asay-Davis +1

Dust at the midplane of a circumstellar disk can become gravitationally unstable and fragment into planetesimals if the local dust-to-gas density ratio mu is sufficiently high. We…

astro-ph.EP2010★ 43 cited

Forming Planetesimals by Gravitational Instability: I. The Role of the Richardson Number in Triggering the Kelvin-Helmholtz Instability

Aaron T. Lee, Eugene Chiang, Xylar Asay-Davis +1

Gravitational instability (GI) of a dust-rich layer at the midplane of a gaseous circumstellar disk is one proposed mechanism to form planetesimals, the building blocks of rocky pl…