Parallel tracks as quasi-steady states for the magnetic boundary layers in neutron-star low-mass X-ray binaries
M. Hakan Erkut, Onur \c{C}atmabacak

TL;DR
This paper models the magnetic boundary layer in neutron-star low-mass X-ray binaries to explain the observed parallel tracks in kHz QPO frequency versus flux, revealing quasi-steady states influenced by boundary layer dynamics.
Contribution
It introduces a boundary region model for kHz QPOs that reproduces parallel tracks and explains their long-term evolution in neutron-star LMXBs.
Findings
Parallel tracks correspond to quasi-steady states of the boundary layer.
Radial width of the boundary layer varies with flux evolution.
A generic model describes the average steady behavior of the boundary region.
Abstract
The neutron stars in low-mass X-ray binaries (LMXBs) are usually thought to be weakly magnetized objects accreting matter from their low-mass companions in the form of a disk. Albeit weak as compared to those in young neutron-star systems, the neutron-star magnetospheres in LMXBs can play an important role in determining the correlations between spectral and temporal properties. Parallel tracks appearing in the plane of kilohertz (kHz) quasi-periodic oscillation (QPO) frequency versus X-ray flux can be used as a tool to study the magnetosphere-disk interaction in neutron-star LMXBs. For dynamically important weak fields, the formation of a non-Keplerian magnetic boundary layer at the innermost disk truncated near the surface of the neutron star is highly likely. Such a boundary region may harbor oscillatory modes of frequencies in the kHz range. We generate parallel tracks using the…
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