Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers Posted on December 21, 2017 by pau
Revealing the formation of stellar-mass black hole binaries: The need for deci-Hertz gravitational wave observatories Posted on March 1, 2017March 1, 2017 by pau
The distribution of stars around the Milky Way’s black hole III: Comparison with simulations Posted on March 1, 2017March 1, 2017 by pau
The distribution of stars around the Milky Way’s central black hole II: Diffuse light from sub-giants and dwarfs Posted on March 1, 2017March 1, 2017 by pau
The distribution of old stars around the Milky Way’s central black hole I: Star counts Posted on March 1, 2017March 1, 2017 by pau
Hybrid methods in planetesimal dynamics: Formation of protoplanetary systems and the mill condition Posted on March 14, 2016 by pau
