activity
19992012
most citedFast coalescence of massive black hole binaries from mergers of galactic nuclei: implications for low-frequency gravitational-wave astrophysics

181 citations · 912 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2012★ 111 cited

Mergers of Unequal Mass Galaxies: Supermassive Black Hole Binary Evolution and Structure of Merger Remnants

Fazeel Mahmood Khan, Miguel Preto, Peter Berczik +3

Galaxy centers are residing places for Super Massive Black Holes (SMBHs). Galaxy mergers bring SMBHs close together to form gravitationally bound binary systems which, if able to c…

astro-ph.GA2011★ 181 cited

Fast coalescence of massive black hole binaries from mergers of galactic nuclei: implications for low-frequency gravitational-wave astrophysics

Miguel Preto, Ingo Berentzen, Peter Berczik +1

We investigate a purely stellar dynamical solution to the Final Parsec Problem. Galactic nuclei resulting from major mergers are not spherical, but show some degree of triaxiality.…

astro-ph.CO2010★ 90 cited

The impact of realistic models of mass segregation on the event rate of extreme-mass ratio inspirals and cusp re-growth

Pau Amaro-Seoane, Miguel Preto

One of the most interesting sources of gravitational waves (GWs) for LISA is the inspiral of compact objects on to a massive black hole (MBH), commonly referred to as an "extreme-m…

astro-ph.CO2010

Gravitational Waves Notes, Issue #3 : "Stellar cusps in galactic nuclei - How stars distribute around a massive black hole"

Pau Amaro-Seoane, Bernard Schutz, Miguel Preto

GW Notes was born from the need for a journal where the distinct communities involved in gravitation wave research might gather. While these three communities - Astrophysics, Gener…

astro-ph.GA2009★ 123 cited

On strong mass segregation around a massive black hole: Implications for lower-frequency gravitational-wave astrophysics

Miguel Preto, Pau Amaro-Seoane

We present, for the first time, a clear -body realization of the {\it strong mass segregation} solution for the stellar distribution around a massive black hole. We compare our…

astro-ph.GA2009★ 63 cited

On post-Newtonian orbits and the Galactic-center stars

Miguel Preto, Prasenjit Saha

Stars near the Galactic center reach a few percent of light speed during pericenter passage, which makes post-Newtonian effects potentially detectable. We formulate the orbit equat…