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19952026
most citedDynamics of Protoplanetary Disks

517 citations · 12.3k across the 161 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.EP2013★ 51 cited

The Long-Term Dynamical Evolution of Planetary Systems

Melvyn B. Davies, Fred C. Adams, Philip Armitage +5

This chapter concerns the long-term dynamical evolution of planetary systems from both theoretical and observational perspectives. We begin by discussing the planet-planet interact…

astro-ph.EP2013★ 136 cited

The Dispersal of Protoplanetary Disks

Richard Alexander, Ilaria Pascucci, Sean Andrews +2

Protoplanetary disks are the sites of planet formation, and the evolution and eventual dispersal of these disks strongly influences the formation of planetary systems. Disk evoluti…

astro-ph.EP2013★ 65 cited

Two timescale dispersal of magnetized protoplanetary disks

Philip J. Armitage, Jacob B. Simon, Rebecca G. Martin

Protoplanetary disks are likely to be threaded by a weak net flux of vertical magnetic field that is a remnant of the much larger fluxes present in molecular cloud cores. If this f…

astro-ph.EP2013★ 52 cited

Formation of circumbinary planets in a dead zone

Rebecca G. Martin, Philip J. Armitage, Richard D. Alexander

Circumbinary planets have been observed at orbital radii where binary perturbations may have significant effects on the gas disk structure, on planetesimal velocity dispersion, and…

astro-ph.SR2013★ 191 cited

Turbulence In the Outer Regions of Protoplanetary Disks. II. Strong Accretion Driven by a Vertical Magnetic Field

Jacob B. Simon, Xue-Ning Bai, Philip J. Armitage +2

We carry out a series of local, vertically stratified shearing box simulations of protoplanetary disks that include ambipolar diffusion and a net vertical magnetic field. The ambip…

astro-ph.SR2013★ 104 cited

The interplay between X-ray photoevaporation and planet formation

Giovanni P. Rosotti, Barbara Ercolano, James E. Owen +1

We assess the potential of planet formation instigating the early formation of a photoevaporation driven gap, up to radii larger than typical for photoevaporation alone. For our in…