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20022023
most citedClumps in the Outer Disk by Disk Instability: Why They are Initially Gas Giants and the Legacy of Disruption

267 citations · 1.7k across the 30 of their papers we have counts for

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Showing astro-ph.EPShow all

8 papers · 1 filter

astro-ph.EP2023★ 18 cited

Constraints on the initial mass, age and lifetime of Saturn's rings from viscous evolutions that include pollution and transport due to micrometeoroid bombardment

Paul R. Estrada, Richard. H. Durisen

The Cassini spacecraft provided key measurements during its more than twelve year mission that constrain the absolute age of Saturn's rings. These include the extrinsic micrometeor…

astro-ph.EP2023★ 14 cited

Large mass inflow rates in Saturn's rings due to ballistic transport and mass loading

R. H. Durisen, Paul. R. Estrada

The Cassini mission provided key measurements needed to determine the absolute age of Saturn's rings, including the extrinsic micrometeoroid flux at Saturn, the volume fraction of…

astro-ph.EP2015★ 43 cited

Gravitational instabilities in a protosolar-like disc I: dynamics and chemistry

M. G. Evans, J. D. Ilee, A. C. Boley +4

To date, most simulations of the chemistry in protoplanetary discs have used 1+1D or 2D axisymmetric -disc models to determine chemical compositions within young systems. This a…

astro-ph.EP2011★ 81 cited

Migration of Gas Giant Planets in Gravitationally Unstable Disks

Scott Michael, Richard H. Durisen, Aaron C. Boley

Characterization of migration in gravitationally unstable disks is necessary to understand the fate of protoplanets formed by disk instability. As part of a larger study, we are us…

astro-ph.EP2010★ 18 cited

Giant Planet Formation

Gennaro D'Angelo, Richard H. Durisen, Jack J. Lissauer

Gas giant planets play a fundamental role in shaping the orbital architecture of planetary systems and in affecting the delivery of volatile materials to terrestrial planets in the…

astro-ph.EP2010★ 1 cited

Stellar Motion Induced by Gravitational Instabilities in Protoplanetary Disks

Scott Michael, R. H. Durisen

We test the effect of assumptions about stellar motion on the behavior of gravitational instabilities in protoplanetary disks around solar-type stars by performing two simulations…