activity
19992013
most citedEccentricity of supermassive black hole binaries coalescing from gas rich mergers

198 citations · 479 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2013★ 53 cited

Convergence of simulations of self-gravitating accretion discs II: Sensitivity to the implementation of radiative cooling and artificial viscosity

W. K. M. Rice, S. -J. Paardekooper, D. H. Forgan +1

Recently it has been suggested that the fragmentation boundary in Smoothed Particle Hydrodynamic (SPH) and FARGO simulations of self-gravitating accretion discs with beta-cooling d…

astro-ph.EP2009★ 115 cited

Planet-planet scattering in planetesimal disks

Sean N. Raymond, Philip J. Armitage, Noel Gorelick

We study the final architecture of planetary systems that evolve under the combined effects of planet-planet and planetesimal scattering. Using N-body simulations we investigate th…

astro-ph2008

Eccentricity of masing disks in Active Galactic Nuclei

Philip J. Armitage

Observations of Keplerian disks of masers in NCG 4258 and other Seyfert galaxies can be used to obtain geometric distance estimates and derive the Hubble constant. The ultimate pre…

astro-ph2006★ 48 cited

Predictions for the correlation between giant and terrestrial extrasolar planets in dynamically evolved systems

Dimitri Veras, Philip J. Armitage

The large eccentricities of many giant extrasolar planets may represent the endpoint of gravitational scattering in initially more crowded systems. If so, the early evolution of th…

astro-ph2005★ 198 cited

Eccentricity of supermassive black hole binaries coalescing from gas rich mergers

Philip J. Armitage, Priyamvada Natarajan

Angular momentum loss to circumbinary gas provides a possible mechanism for overcoming the `last parsec' problem and allowing the most massive black hole binaries formed from galac…

astro-ph1999★ 65 cited

Early planet formation as a trigger for further planet formation

Philip J. Armitage, Brad M. S. Hansen

Recent discoveries of extrasolar planets at small orbital radii, or with significant eccentricities, indicate that interactions between massive planets and the disks of gas and dus…