On the kHz QPO frequency correlations in bright neutron star X-ray binaries
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/376/3/1133/4874262/mnras0376-1133.pdf
Reference38 articles.
1. A precise determination of black hole spin in GRO J1655-40
2. Evidence for a 2:3 resonance in Sco X-1 kHz QPOs
3. A Unified Description of the Timing Features of Accreting X‐Ray Binaries
4. The distribution of kHz QPO frequencies in bright low mass X-ray binaries
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1. QPOs in Compact Sources as a Nonlinear Hydrodynamical Resonance: Determining Spin of Compact Objects;The Astrophysical Journal;2023-09-21
2. Parallel tracks of kHz QPOs: implication of the bimodal luminosity components in neutron star low-mass X-ray binaries;Monthly Notices of the Royal Astronomical Society;2023-01-25
3. Simple Analytic Formula Relating the Mass and Spin of Accreting Compact Objects to Their Rapid X-Ray Variability;The Astrophysical Journal;2022-04-01
4. Relation Between the Variability of the Kilo-Hertz Quasi-Periodic Oscillations and the Low-Frequency Noise in $$4U 1608{-}52$$;Springer Proceedings in Physics;2021
5. Models of high-frequency quasi-periodic oscillations and black hole spin estimates in Galactic microquasars;Astronomy & Astrophysics;2020-10-27
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