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20022008
most citedHyperfast pulsars as the remnants of massive stars ejected from young star clusters

47 citations · 55 across the 7 of their papers we have counts for

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astro-ph200868 cited

Explaining the Orbits of the Galactic Center S-Stars

David Merritt, Alessia Gualandris, Seppo Mikkola

The young stars near the supermassive black hole at the galactic center follow orbits that are nearly random in orientation and that have an approximately thermal distribution of e…

astro-ph20081 cited

Dynamical evolution of the young stars in the Galactic center

Hagai. B. Perets, Alessia Gualandris, David Merritt +1

Recent observations of the Galactic center revealed a nuclear disk of young OB stars near the massive black hole (MBH), in addition to many similar outlying stars with higher eccen…

astro-ph200717 cited

A parallel gravitational N-body kernel

Simon Portegies Zwart, Steve McMillan, Derek Groen +3

We describe source code level parallelization for the {\tt kira} direct gravitational -body integrator, the workhorse of the {\tt starlab} production environment for simulating…

astro-ph20076 cited

Dynamics around supermassive black holes

Alessia Gualandris, David Merritt

The dynamics of galactic nuclei reflects the presence of supermassive black holes (SBHs) in many ways. Single SBHs act as sinks, destroying a mass in stars equal to their own mass…

astro-ph2007243 cited

Ejection of Supermassive Black Holes from Galaxy Cores

Alessia Gualandris, David Merritt

[Abridged] Recent numerical relativity simulations have shown that the emission of gravitational waves during the merger of two supermassive black holes (SMBHs) delivers a kick to…

astro-ph200737 cited

On the onset of runaway stellar collisions in dense star clusters I. Dynamics of the first collision

E. Gaburov, A. Gualandris, S. Portegies Zwart

We study the circumstances under which first collisions occur in young and dense star clusters. The initial conditions for our direct -body simulations are chosen such that the…