Sharp eccentric rings in planetless hydrodynamical models of debris disks
Wladimir Lyra, Marc J. Kuchner

TL;DR
This study uses 2D hydrodynamical models to show that gas-dust interactions can naturally produce eccentric rings in debris disks, challenging the need to invoke unseen planets as the cause.
Contribution
The paper demonstrates that gas-dust hydrodynamics can generate eccentric rings and standing wave oscillations, providing an alternative explanation to planetary influences.
Findings
Gas-dust backreaction shepherds rings similar to observed debris disks.
Eccentricity of rings can be explained by standing wave oscillations.
Eccentric rings do not necessarily imply the presence of planets.
Abstract
Debris disks should not be completely gas-free, since there is second generation gas from outgassing of planetesimals and dust grains via sublimation, photodesorption, or collisions, generating a system of dust-to-gas ratio close to unity, where hydrodynamics cannot be ignored. A clumping instability exists in this configuration, that has been hitherto explored only in one-dimensional, incompressible models. We performed 2D numerical compressible models of a disk with comparable amounts of gas and dust to study the growth and development of this instability. Our model solves the momentum equation for the gas and dust, together with energy and continuity equations. We uncover that the backreaction of the drag force from the gas onto the dust shepherds rings, similar to those observed in debris disks and usually attributed to the presence of hypothetical undetected planets. We also…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Astro and Planetary Science · High-pressure geophysics and materials
