A Temporal Scale to Track the Spectral Transitions in Low-Mass X-ray Binaries
E. Sonbas, K. Mohamed, K. S. Dhuga, E. G\"o\u{g}\"u\c{s}

TL;DR
This study introduces a temporal scale based on wavelet analysis to track spectral transitions in low-mass X-ray binaries, revealing potential markers to distinguish black hole and neutron star systems.
Contribution
It develops a novel minimal time scale metric from high-resolution lightcurves to compare spectral state evolution in LMXBs, aiding in source classification.
Findings
High fractional RMS and hardness correlate with both BH and NS sources.
Atolls show large MTS, Z-type sources show small MTS at low RMS.
BH sources occupy a unique low-hardness, small-MTS region in the hardness-MTS plane.
Abstract
The results of a temporal analysis of observations for a sample of nine low-mass X-ray binaries (LMXBs) are presented. Of these sources, five host a neutron star (NS) primary (4U1608-52, Aql X-1, 4U1705-44, GX17+2 and Cyg X-2), and four host a black hole (BH) (GX339-4, XTE J1859+226, H1743-322 and MAXI J1659-152). The NS group includes three Atolls and two Z-type sources. We utilized archival Proportional Counter Array (PCA)/RXTE data to construct high-resolution lightcurves. A wavelet transform of the lightcurves is deployed to extract a minimal time scale (MTS) associated with the spectral state of the sources. The MTS, together with the fractional root-mean-square (RMS) and hardness ratios, is used to construct RMS-MTS and hardness-MTS diagrams that enable a direct comparison of the evolution of spectral transitions in the target sources. Observations with high fractional RMS and…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Astronomy and Astrophysical Research
