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20012011
most citedIntermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

583 citations · 922 across the 12 of their papers we have counts for

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11 papers · 1 filter

astro-ph2007583 cited

Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

Pau Amaro-Seoane, Jonathan R. Gair, Marc Freitag +4

Black hole binaries with extreme () or intermediate () mass ratios are among the most interesting gravitational wave sources that are expected to…

astro-ph20067 cited

Gravitational waves from coalescing massive black holes in young dense clusters

Pau Amaro-Seoane

HST observations reveal that young massive star clusters form in gas-rich environments like the Antennæ galaxy which will merge in collisional processes to form larger structures.…

astro-ph200673 cited

Intermediate-mass black holes in colliding clusters: Implications for lower-frequency gravitational-wave astronomy

Pau Amaro-Seoane, Marc Freitag

Observations suggest that star clusters often form in binaries or larger bound groups. Therefore, mergers between two clusters are likely to occur. If these clusters both harbor an…

astro-ph200613 cited

The MODEST questions: challenges and future directions in stellar cluster research

Melvyn B. Davies, Pau Amaro-Seoane, Cees Bassa +7

We present a review of some of the current major challenges in stellar cluster research, including young clusters, globular clusters, and galactic nuclei. Topics considered include…

astro-ph200696 cited

A comprehensive Nbody study of mass segregation in star clusters: Energy equipartition and escape

Emil Khalisi, Pau Amaro-Seoane, Rainer Spurzem

We address the dynamical evolution of an isolated self--gravitating system with two stellar mass groups. We vary the individual ratio of the heavy to light bodies, from 1.25 to…

astro-ph200670 cited

Dynamics of compact objects clusters: A post-Newtonian study

Gabor Kupi, Pau Amaro-Seoane, Rainer Spurzem

Compact object clusters are likely to exist in the centre of some galaxies because of mass segregation. The high densities and velocities reached in them deserves a better understa…