Models of QPOs in luminous low-mass X-ray binaries
- 1 January 1988
- journal article
- Published by Elsevier in Advances In Space Research
- Vol. 8 (2) , 421-447
- https://doi.org/10.1016/0273-1177(88)90440-1
Abstract
No abstract availableKeywords
This publication has 32 references indexed in Scilit:
- A new example of the Papaloizou-Pringle instabilityThe Astrophysical Journal, 1987
- Coherence effects on quasi-periodic oscillations from Galactic X-ray sourcesThe Astrophysical Journal, 1987
- Effect of an electron scattering cloud on X-ray oscillations produced by beamingThe Astrophysical Journal, 1987
- Model QPO power spectra: signatures of angular position and radial velocity of clumps in the boundary layerMonthly Notices of the Royal Astronomical Society, 1986
- Quasi-periodic oscillations from accretion disk coronasNature, 1986
- A model for quasi-periodic oscillations in low-mass X-ray binariesNature, 1985
- Is GX5 – 1 a millisecond pulsar?Nature, 1985
- Techniques for the estimation of red power spectra. II Evaluation of alternative methodsThe Astrophysical Journal, 1984
- Accretion by rotating magnetic neutron stars. III - Accretion torques and period changes in pulsating X-ray sourcesThe Astrophysical Journal, 1979
- Accretion by rotating magnetic neutron stars. II - Radial and vertical structure of the transition zone in disk accretionThe Astrophysical Journal, 1979