activity
19982016
most citedRossby Wave Instability of Keplerian Accretion Disks

621 citations · 1.5k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2016★ 29 cited

Dynamics of Circumstellar Disks III: The case of GG Tau A

Andrew F. Nelson, F. Marzari

(abridged) We present 2-dimensional hydrodynamic simulations using the Smoothed Particle Hydrodynamic (SPH) code, VINE, to model a self-gravitating binary system similar to the GG…

astro-ph.EP2012★ 6 cited

Dynamics of Core Accretion

Andrew F. Nelson, Maximilian Ruffert

(shortened) We perform 3D hydrodynamic simulations of gas flowing around a planetary core of mass \mplan=10\me embedded in a near Keplerian background flow, using a modified sheari…

astro-ph.EP2009★ 60 cited

Interaction of a giant planet in an inclined orbit with a circum-stellar disk

F. Marzari, Andrew F. Nelson

We investigate the dynamical evolution of a Jovian--mass planet injected into an orbit highly inclined with respect to its nesting gaseous disk. Planet--planet scattering induced b…

astro-ph2008★ 42 cited

VINE -- A numerical code for simulating astrophysical systems using particles II: Implementation and performance characteristics

Andrew F. Nelson, M. Wetzstein, T. Naab +1

We continue our presentation of VINE. We begin with a description of relevant architectural properties of the serial and shared memory parallel computers on which VINE is intended…

astro-ph2008★ 71 cited

VINE -- A numerical code for simulating astrophysical systems using particles I: Description of the physics and the numerical methods

M. Wetzstein, Andrew F. Nelson, T. Naab +1

We present a Fortran 95 code for simulating the evolution of astrophysical systems using particles to represent the underlying fluid flow. The code is designed to be versatile, fle…

astro-ph2007★ 1 cited

Gravitational instability in binary protoplanetary disks

Lucio Mayer, Alan Boss, Andrew F. Nelson

We review the models and results of simulations of self-gravitating, gaseous protoplanetary disks in binary star systems. These models have been calculated by three different group…