Kelly Holley-Bockelmann

Chandra and XMM-Newton Observations of the Abell 3395/Abell 3391 Intercluster Filament

We present Chandra and XMM-Newton X-ray observations of the Abell 3391/Abell 3395 intercluster filament. It has been suggested that the galaxy clusters Abell 3395, Abell 3391, and the galaxy group ESO-161 located between the two clusters, are in alignment along a large-scale intercluster filament. We find that the filament is aligned close to the plane of the sky, in contrast to previous results. We find a global projected filament temperature kT =

The Evolution of Cuspy Triaxial Galaxies Harboring Central Black Holes

4.45_{-0.55}^{+0.89}

MODELS OF CUSPY TRIAXIAL GALAXIES

~keV, electron density

A full loss cone for triaxial galaxies

n_e=1.08^{+0.06}_{-0.05} \times 10^{-4}

Hypervelocity intracluster stars ejected by supermassive black hole binaries

~cm

Survivability of Realistic Satellite Galaxies Near Host Galaxies

^{-3}

The Synthetic Galaxy: Double Compact Object Populations.

, and

An Imaging Survey of Satellite Galaxies

M_{\rm gas} = 2.7^{+0.2}_{-0.1} \times 10^{13}

Gravitational Waves From The Hierarchical Buildup Of Intermediate Mass Black Holes

~M

N-body Simulations of the Assembly History of Supermassive Black Holes

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