The timing properties of Sco X-1 along its Z track with EXOSAT
Open Access
- 1 January 2000
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 311 (1) , 201-224
- https://doi.org/10.1046/j.1365-8711.2000.03050.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 39 references indexed in Scilit:
- Ocean g-Modes on Rotating Neutron StarsThe Astrophysical Journal, 1996
- Nonradial Oscillations in Neutron Star Oceans: A Source of Quasi-periodic X-Ray Oscillations?The Astrophysical Journal, 1995
- Propagation of nuclear burning fronts on accreting neutron stars: X-ray bursts and sub-hertz noiseThe Astrophysical Journal, 1995
- X-ray variability of Scorpius X-1 during a multiwavelength campaignThe Astrophysical Journal, 1992
- Origin of 'normal-branch' quasiperiodic oscillations in low-mass X-ray binary systemsNature, 1989
- A third X-ray spectral mode in Scorpius X-1 - Similarities to the other bright bulge sourcesThe Astrophysical Journal, 1989
- Quasi-periodic oscillations in the X-ray flux of Cyg X-2Nature, 1986
- Is GX5 – 1 a millisecond pulsar?Nature, 1985
- Techniques for the estimation of red power spectra. II Evaluation of alternative methodsThe Astrophysical Journal, 1984
- Evidence for x Rays From Sources Outside the Solar SystemPhysical Review Letters, 1962