A model-independent comparison of the variability of accreting neutron stars and black holes

Abstract

We use Rossi X-ray Timing Explorer observations to conduct a population study of the timing properties of accretion-powered neutron star Low Mass X-ray Binaries (LMXBs), following a model-independent approach that was originally applied to black hole systems. The ratios of integrated power in four equally spaced Fourier frequency bands allow power spectral shapes to be parameterised with two `power colour' values, providing a simple way of tracking the evolution in timing properties across observations. We show that neutron star LMXBs follow a remarkably similar power spectral evolution to black hole LMXBs, confirming that the broadband noise variability seen in both types of system has a common origin in the accretion flow. Both neutron stars and black holes follow a similar clear track in the power colour-colour diagram as they transition from the hard through soft states. Quantifying the position on this oval track using a single parameter, the power-spectral `hue', we find that the transition in X-ray spectral shape occurs at the same hue for both neutron star and black hole systems. The power colours of Z sources map on to those of soft state black holes, while those of atoll sources correspond to all spectral states. There is no clear dependence of power colour on neutron star spin, or on whether the neutron star is clearly magnetised (determined by ms X-ray pulsations).

21 pages, 19 figures, accepted for publication in MNRAS

References in corpus (14)

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• The peculiar variable X-ray spectrum of the active galactic nucleus PKS 2005-489
• Evolution of MAXI J1631-479 during the January 2019 outburst observed by INTEGRAL/IBIS
• A Temporal Scale to Track the Spectral Transitions in Low-Mass X-ray Binaries
• QPOML: A Machine Learning Approach to Detect and Characterize Quasi-Periodic Oscillations in X-ray Binaries
• Multi-band power color-color diagrams of three black hole X-ray binaries observed with Insight-HXMT