activity
20242026
collaborators

11 papers

astro-ph.HE2026

Tilted, warped, and eccentric disks

P. Chris Fragile, Adam Ingram, Gibwa Musoke +1

We review some of the interesting consequences that tilts, warps, and eccentricities can introduce into the dynamics, thermodynamics, and observational appearance of accreting syst…

astro-ph.EP2025

Non-linear spiral waves in accretion discs

Joshua J. Brown, Gordon I. Ogilvie

We derive a simple, accurate, non-linear, global equation governing spiral density waves in thin, non-self-gravitating, inviscid accretion discs. These discs may have any slowly va…

astro-ph.SR2025

Disc breaking and parametric instability in warped accretion discs

Loren E Held, Gordon I. Ogilvie

We present the first local simulations of disc breaking/tearing in a warped accretion disc. Warps can arise due to a misalignment between the disc and the rotation axis of the cent…

astro-ph.SR2025

Instability and vertical eccentricity variation in global hydrodynamic disk simulations

Janosz W. Dewberry, Henrik N. Latter, Gordon I. Ogilvie +1

Many dynamical interactions can induce eccentricities in astrophysical accretion disks. Disk eccentricities in turn seed a variety of instabilities, even in ideal hydrodynamics. We…

astro-ph.EP2025

High-resolution models of the vertical shear instability

Geoffroy Lesur, Henrik N. Latter, Gordon I. Ogilvie

(abridged) Context: The vertical shear instability (VSI) is a promising mechanism to generate turbulence and transport angular momentum in protoplanetary discs. While most recent w…

astro-ph.EP2025

The Laplace Surface of a Circumplanetary Disc

Stephen H. Lubow, Gordon I. Ogilvie

The classical Laplace surface defines the location of circular particle orbits that do not undergo nodal precession around a planet with some obliquity. Close to the planet the sur…