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19982022
most citedProduction of Intermediate-Mass Black Holes in Globular Clusters

493 citations · 3.4k across the 43 of their papers we have counts for

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12 papers · 1 filter

astro-ph2008★ 82 cited

Intermediate Mass Black Hole Induced Quenching of Mass Segregation in Star Clusters

Michael Gill, Michele Trenti, M. Coleman Miller +3

In many theoretical scenarios it is expected that intermediate-mass black holes (IMBHs, with masses M ~ 100-10000 solar masses) reside at the centers of some globular clusters. How…

astro-ph2008★ 26 cited

Galileo In-Situ Dust Measurements in Jupiter's Gossamer Rings

Harald Krueger, Douglas P. Hamilton, Richard Moissl +1

During its late orbital mission at Jupiter the Galileo spacecraft made two passages through the giant planet's gossamer ring system. The impact-ionization dust detector on board su…

astro-ph2005★ 143 cited

Three-Body Dynamics with Gravitational Wave Emission

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

We present numerical three-body experiments that include the effects of gravitational radiation reaction by using equations of motion that include the 2.5-order post-Newtonian forc…

astro-ph2005★ 138 cited

Binary Encounters With Supermassive Black Holes: Zero-Eccentricity LISA Events

M. Coleman Miller, Marc Freitag, Douglas P. Hamilton +1

Current simulations of the rate at which stellar-mass compact objects merge with supermassive black holes (called extreme mass ratio inspirals, or EMRIs) focus on two-body capture…

astro-ph2004★ 148 cited

Growth of Intermediate-Mass Black Holes in Globular Clusters

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

We present results of numerical simulations of sequences of binary-single scattering events of black holes in dense stellar environments. The simulations cover a wide range of mass…

astro-ph2003★ 14 cited

Three-Body Encounters of Black Holes in Globular Clusters

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

Evidence has been mounting for the existence of black holes with masses from 10^2 to 10^4 M_Solar associated with stellar clusters. Such intermediate-mass black holes (IMBHs) will…