14 citations · 14 across the 1 of their papers we have counts for
6 papers
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…
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,…
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…
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…
Sonic-Point Model for High-Frequency QPOs in Neutron Star Low-Mass X-Ray Binaries
M. Coleman Miller, Frederick K. Lamb, Dimitrios Psaltis
Quasi-periodic brightness oscillations (QPOs) with frequencies in the range 300-1200 Hz have been detected from at least nine neutron star low-mass X-ray binaries. Here we summariz…
GRO J1744-28: Last Gasps of a Dying Low-mass X-ray Binary
D. Q. Lamb, M. Coleman Miller, R. E. Taam
We argue that the bursting, transient X-ray source GRO J1744-28 is a binary consisting of a very low-mass ($M \approx 0.2 M_\sun$), highly evolved giant star that is transferring m…