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20082025
most citedA Characteristic Scale for Cold Gas

260 citations · 1.1k across the 35 of their papers we have counts for

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Showing astro-ph.EPShow all

8 papers · 1 filter

astro-ph.EP2024★ 1 cited

Tidal Disruption of Planetesimals from an Eccentric Debris Disk Following a White Dwarf Natal Kick

Tatsuya Akiba, Selah McIntyre, Ann-Marie Madigan

The surfaces of many white dwarfs are polluted by metals, implying a recent accretion event. The tidal disruption of planetesimals is a viable source of white dwarf pollution and o…

astro-ph.EP2023★ 2 cited

Steeper Scattered Disks Buckle Faster

Alexander Zderic, Ann-Marie Madigan

Disks of low-mass bodies scattered by giant planets to large semi-major axis and constant periapsis orbits are vulnerable to a buckling instability. This instability exponentially…

astro-ph.EP2021★ 4 cited

A Lopsided Outer Solar System

Alexander Zderic, Maria Tiongco, Angela Collier +3

Axisymmetric disks of eccentric orbits in near-Keplerian potentials are unstable to an out-of-plane buckling. Recently, Zderic et al. (2020) showed that an idealized disk saturates…

astro-ph.EP2020★ 10 cited

Giant Planet Influence on the Collective Gravity of a Primordial Scattered Disk

Alexander Zderic, Ann-Marie Madigan

Axisymmetric disks of high eccentricity, low mass bodies on near-Keplerian orbits are unstable to an out-of-plane buckling. This "inclination instability" exponentially grows the o…

astro-ph.EP2020★ 8 cited

Apsidal Clustering following the Inclination Instability

Alexander Zderic, Angela Collier, Maria Tiongco +1

Disks of low-mass bodies on high-eccentricity orbits in near-Keplerian potentials can be dynamically unstable to buckling out of the plane. In this letter, we present -body simu…

astro-ph.EP2019★ 3 cited

Secular Eccentricity Oscillations in Axisymmetric Disks of Eccentric Orbits

Jacob Fleisig, Alexander Zderic, Ann-Marie Madigan

Massive bodies undergo orbital eccentricity oscillations when embedded in an axisymmetric disk of smaller mass orbits. These eccentricity oscillations are driven by secular torques…

astro-ph.EP2018★ 16 cited

On the Dynamics of the Inclination Instability

Ann-Marie Madigan, Alexander Zderic, Michael McCourt +1

Axisymmetric disks of eccentric Kepler orbits are vulnerable to an instability which causes orbits to exponentially grow in inclination, decrease in eccentricity, and cluster in th…

astro-ph.EP2015★ 57 cited

A new inclination instability reshapes Keplerian disks into cones: application to the outer Solar System

Ann-Marie Madigan, Michael McCourt

Disks of bodies orbiting a much more massive central object are extremely common in astrophysics. When the orbits comprising such disks are eccentric, we show they are susceptible…