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20082025
most citedAthena: A New Code for Astrophysical MHD

974 citations · 4.5k across the 46 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2020★ 180 cited

Measuring turbulent motion in planet-forming disks with ALMA: A detection around DM Tau and non-detections around MWC 480 and V4046 Sgr

Kevin Flaherty, A. Meredith Hughes, Jacob B. Simon +6

Turbulence is a crucial factor in many models of planet formation, but it has only been directly constrained among a small number of planet forming disks. Building on the upper lim…

astro-ph.SR2018★ 3 cited

The Nature of Turbulence in the Outer Regions of Protoplanetary Disks

Daniel A. Gole, Jacob B. Simon

We carry out a series of local, shearing box simulations of the outer regions of protoplanetary disks, where ambipolar diffusion is important due to low ionization levels, to bette…

astro-ph.SR2017★ 52 cited

Origin of Weak Turbulence in the Outer Regions of Protoplanetary Disks

Jacob B. Simon, Xue-Ning Bai, Kevin M. Flaherty +1

The mechanism behind angular momentum transport in protoplanetary disks, and whether this transport is turbulent in nature, is a fundamental issue in planet formation studies. Rece…

astro-ph.SR2016★ 14 cited

Turbulence, Transport and Waves in Ohmic Dead Zones

Daniel Gole, Jacob B. Simon, Stephen H. Lubow +1

We use local numerical simulations to study a vertically stratified accretion disk with a resistive mid-plane that damps magnetohydrodynamic (MHD) turbulence. This is an idealized…

astro-ph.SR2015★ 344 cited

The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. I. The Role of Self-Gravity

Jacob B. Simon, Philip J. Armitage, Rixin Li +1

We study the formation of planetesimals in protoplanetary disks from the gravitational collapse of solid over-densities generated via the streaming instability. To carry out these…

astro-ph.SR2015★ 168 cited

Magnetically driven accretion in protoplanetary discs

Jacob B. Simon, Geoffroy Lesur, Matthew W. Kunz +1

We characterize magnetically driven accretion at radii between 1 au and 100 au in protoplanetary discs, using a series of local non-ideal magnetohydrodynamic (MHD) simulations. The…