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20052016
most citedGravitational waves from scattering of stellar-mass black holes in galactic nuclei

523 citations · 2.5k across the 23 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 51 cited

Star Clusters Around Recoiled Black Holes in the Milky Way Halo

Ryan M. O'Leary, Abraham Loeb

Gravitational wave emission by coalescing black holes (BHs) kicks the remnant BH with a typical velocity of hundreds of km/s. This velocity is sufficiently large to remove the remn…

astro-ph2008★ 523 cited

Gravitational waves from scattering of stellar-mass black holes in galactic nuclei

Ryan M. O'Leary, Bence Kocsis, Abraham Loeb

Stellar mass black holes (BHs) are expected to segregate and form a steep density cusp around supermassive black holes (SMBHs) in galactic nuclei. We follow the evolution of a mult…

astro-ph2007★ 41 cited

Hypervelocity Stars from the Andromeda Galaxy

Blake D. Sherwin, Abraham Loeb, Ryan M. O'Leary

Hypervelocity stars (HVSs) discovered in the Milky Way (MW) halo are thought to be ejected from near the massive black hole (MBH) at the galactic centre. In this paper we investiga…

astro-ph2007★ 67 cited

Dynamical Interactions and the Black Hole Merger Rate of the Universe

Ryan O'Leary, Richard O'Shaughnessy, Frederic Rasio

Binary black holes can form efficiently in dense young stellar clusters, such as the progenitors of globular clusters, via a combination of gravitational segregation and cluster ev…

astro-ph2006★ 69 cited

Production of Hypervelocity Stars through Encounters with Stellar-Mass Black Holes in the Galactic Centre

Ryan M. O'Leary, Abraham Loeb

Stars within 0.1 pc of the supermassive black hole Sgr A* at the Galactic centre are expected to encounter a cluster of stellar-mass black holes (BHs) that have segregated to that…

astro-ph2005★ 324 cited

Binary Mergers and Growth of Black Holes in Dense Star Clusters

Ryan M. O'Leary, Frederic A. Rasio, John M. Fregeau +2

We model the dynamical evolution of primordial black holes (BHs) in dense star clusters using a simplified treatment of stellar dynamics in which the BHs are assumed to remain conc…