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19962007
most citedModeling kicks from the merger of non-precessing black-hole binaries

132 citations · 192 across the 3 of their papers we have counts for

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astro-ph2007132 cited

Modeling kicks from the merger of non-precessing black-hole binaries

John G. Baker, William D. Boggs, Joan Centrella +4

Several groups have recently computed the gravitational radiation recoil produced by the merger of two spinning black holes. The results suggest that spin can be the dominant contr…

astro-ph200746 cited

Supporting evidence for the signature of the innermost stable circular orbit in Rossi X-ray data from 4U1636-536

Didier Barret, Jean-Francois Olive, M. Coleman Miller

Analysis of archival RXTE data on neutron stars binaries has shown that for several sources the quality factor (Q) of the lower kilohertz Quasi-Periodic Oscillations (QPO) drops sh…

astro-ph200314 cited

Sonic-Point and Spin-Resonance Model of the Kilohertz QPO Pairs

Frederick K. Lamb, M. Coleman Miller

KHz QPOs have now been detected in more than twenty accreting neutron stars in low-mass binary systems. Two kHz QPOs are usually detected in each star. Burst oscillations and two k…

astro-ph1998

The Origin of Kilohertz QPOs and Implications for Neutron Stars

Frederick K. Lamb, M. Coleman Miller, Dimitrios Psaltis

One of the most dramatic discoveries made with the Rossi X-Ray Timing Explorer is that many accreting neutron stars in low-mass binary systems produce strong, remarkably coherent,…

astro-ph1998

Constraints on neutron star matter from kilohertz QPOs

F. K. Lamb, M. C. Miller, D. Psaltis

One of the most dramatic discoveries made so far with the Rossi X-Ray Timing Explorer is that many accreting neutron stars with weak magnetic fields generate strong, remarkably coh…

astro-ph1997

Models of Kilohertz Quasi-Periodic Brightness Oscillations

M. Coleman Miller

The remarkable discovery of kilohertz quasi-periodic brightness oscillations (QPOs) in the accretion-powered emission from some sixteen neutron-star low-mass X-ray binary systems h…