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20032018
most citedGiant Planet Formation by Disk Instability: A Comparison Simulation With An Improved Radiative Scheme

45 citations · 79 across the 5 of their papers we have counts for

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5 papers

astro-ph.SR2018★ 6 cited

A 3D Hydrodynamics Study of Gravitational Instabilities in a Young Circumbinary Disc

Karna M. Desai, Thomas Y. Steiman-Cameron, Scott Michael +2

We present a 3D hydrodynamics study of gravitational instabilities (GIs) in a 0.14 M circumbinary protoplanetary disc orbiting a 1 M star and a 0.02 M…

astro-ph.SR2010★ 27 cited

Confronting 3 Dimensional Time-dependent Jet Simulations with HST Observations

Jan Staff, Brian Niebergal, Rachid Ouyed +2

We perform state-of-the-art, 3D, time-dependent simulations of magnetized disk winds, carried out to simulation scales of 60 Astronomical Units, in order to confront optical HST ob…

astro-ph.SR2009★ 45 cited

Giant Planet Formation by Disk Instability: A Comparison Simulation With An Improved Radiative Scheme

Kai Cai, Megan K. Pickett, Richard H. Durisen +1

There has been disagreement currently about whether cooling in protoplanetary disks can be sufficiently fast to induce the formation of gas giant protoplanets via gravitational ins…

astro-ph2005★ 1 cited

The Effects of Metallicity and Grain Size on Gravitational Instabilities in Protoplanetary Disks

Kai Cai, Richard H. Durisen, Scott Michael +4

Observational studies show that the probability of finding gas giant planets around a star increases with the star's metallicity. Our latest simulations of disks undergoing gravita…

astro-ph2003

A Possible Hybrid Scenario for Gas Giant Planet Formation in Rings

Richard H. Durisen, Kai Cai, Annie C. Mejia +1

The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable gas disk lifetimes, but it has yet to be firmly esta…