activity
20112015
most citedTidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations

59 citations · 157 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2015★ 9 cited

Unveiling Gargantua: A new search strategy for the most massive central cluster black holes

Michael Brockamp, Holger Baumgardt, Silke Britzen +1

We aim to unveil the most massive central cluster black holes in the universe. We present a new search strategy which is based on a black hole mass gain sensitive 'calorimeter' and…

astro-ph.SR2014★ 26 cited

The Puzzling Negative Orbit-Period Derivative of the Low-Mass X-Ray Binary 4U 1820-30 in NGC 6624

Miklos Peuten, Michael Brockamp, Andreas H. W. Kuepper +1

4U 1820-30 is a low-mass X-ray binary near the center of the globular cluster NGC 6624 consisting of, at least, one neutron star and one helium white dwarf. Analyzing 16 years of d…

astro-ph.GA2014★ 13 cited

How tidal erosion has shaped the relation between globular cluster specific frequency and galaxy luminosity

Steffen Mieske, Andreas Kuepper, Michael Brockamp

We quantify to what extent tidal erosion of globular clusters (GCs) has contributed to the observed u-shaped relation between GC specific frequencies S_N and host galaxy luminosity…

astro-ph.GA2014★ 50 cited

Erosion of Globular Cluster Systems: The Influence of Radial Anisotropy, Central Black Holes and Dynamical Friction

Michael Brockamp, Andreas H. W. Kuepper, Ingo Thies +2

We present the adaptable MUESLI code for investigating dynamics and erosion processes of globular clusters (GCs) in galaxies. MUESLI follows the orbits of individual clusters and a…

astro-ph.GA2011★ 59 cited

Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations

M. Brockamp, H. Baumgardt, P. Kroupa

The disruption rate of stars by supermassive black holes (SMBHs) is calculated numerically with a modified version of Aarseth's NBODY6 code. The initial stellar distribution around…