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20012026
most citedThe Evolution of Binary Fractions in Globular Clusters

210 citations · 1.1k across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2026

Empirical determination of the Galactic neutron star--black hole merger rate using StarTrack models

Terrence Pierre Jacques, D. R. Lorimer, Nihan Pol +2

The discovery of a pulsar in a binary system with a black hole would provide a unique laboratory for testing general relativity in the strong-field regime and offer vital constrain…

astro-ph.HE2020★ 2 cited

A supernova remnant associated with a nascent black hole low-mass X-ray binary

N. I. Maxted, A. J. Ruiter, K. Belczynski +2

Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observ…

gr-qc2014

Prospects for Detection of Extragalactic Stellar Black Hole Binaries in the Nearby Universe

Matthew Benacquista, Jesus Hinojosa, Alberto Mata +1

Stellar mass black hole binaries have individual masses between 10-80 solar masses. These systems may emit gravitational waves at frequencies detectable at Megaparsec distances by…

astro-ph.SR2014★ 147 cited

Stellar Mergers Are Common

C. S. Kochanek, Scott M. Adams, Krzysztof Belczynski

The observed Galactic rate of stellar mergers or the initiation of common envelope phases brighter than M_V=-3 (M_I=-4) is of order 0.5 (0.3)/year with 90% confidence statistical u…

astro-ph.SR2012★ 133 cited

On the brightness distribution of Type Ia supernovae from violent white dwarf mergers

A. J. Ruiter, S. A. Sim, R. Pakmor +8

We investigate the brightness distribution expected for thermonuclear explosions that might result from the ignition of a detonation during the violent merger of white dwarf (WD) b…

astro-ph.SR2010★ 4 cited

Type Ia Supernovae and Accretion Induced Collapse

A. J. Ruiter, K. Belczynski, S. A. Sim +3

Using the population synthesis binary evolution code StarTrack, we present theoretical rates and delay times of Type Ia supernovae arising from various formation channels. These ch…