We review the current knowledge about nuclear star clusters (NSCs), the spectacularly dense and massive assemblies of stars found at the centers of most galaxies. Recent …
H Tagawa, Z Haiman, B Kocsis - The Astrophysical Journal, 2020 - iopscience.iop.org
The astrophysical origin of gravitational wave (GW) events discovered by LIGO/VIRGO remains an outstanding puzzle. In active galactic nuclei (AGNs), compact-object binaries …
LAC Van Son, SE De Mink, T Callister… - The Astrophysical …, 2022 - iopscience.iop.org
Gravitational-wave detectors are starting to reveal the redshift evolution of the binary black hole (BBH) merger rate, R BBH (z). We make predictions for R BBH (z) as a function of black …
LAC van Son, SE de Mink, M Renzo… - The Astrophysical …, 2022 - iopscience.iop.org
Gravitational-wave (GW) detections are starting to reveal features in the mass distribution of double compact objects. The lower end of the black hole (BH) mass distribution is especially …
The recently discovered gravitational wave sources GW190521 and GW190814 have shown evidence of BH mergers with masses and spins outside of the range expected from …
There is some weak evidence that the black hole merger named GW190521 had a non-zero eccentricity,. In addition, the masses of the component black holes exceeded the limit …
Primordial black holes (PBHs) might be formed in the early Universe and could comprise at least a fraction of the dark matter. Using the recently released GWTC-2 dataset from the third …
Upcoming observational runs of the LIGO-Virgo-KAGRA Collaboration and future gravitational-wave (GW) detectors on the ground and in space require waveform models …
We present a set of 148 independent N-body simulations of globular clusters (GCs) computed using the code CMC (Cluster Monte Carlo). At an age of∼ 10–13 Gyr, the …