Long-term evolution of Cyclotron Line energy in an eclipsing pulsar 4U 1538-522
Ruchi Tamang, Manoj Ghising, Mohammed Tobrej, Binay Rai, Bikash, Chandra Paul

TL;DR
This study analyzes long-term timing and spectral data of the eclipsing pulsar 4U 1538-522, revealing a complex evolution of its spin, pulse profile, and cyclotron line energy, including a torque reversal and a linear increase in cyclotron energy over time.
Contribution
It provides the first comprehensive analysis of the long-term evolution of the cyclotron line energy and spin behavior in 4U 1538-522 using NuSTAR data, highlighting a torque reversal and spectral changes.
Findings
Spin-down rate of 0.163 s/yr until torque reversal
Cyclotron line energy increased then decreased, with a net increase of 0.08 keV/yr
Pulse profile transitioned from double to single peak above 30 keV
Abstract
We present the timing and spectral analysis of the HMXB source 4U 1538-522 using NuSTAR observations. One of the observations partially covers the X-ray eclipse of the source along with eclipse ingress. The source is found to spin down at the rate of 0.163 0.002 s between (54973-58603) MJD. It is evident that at time 58620 MJD, a torque reversal occurred, thereafter the source exhibited a spin-up trend at the rate - (0.305 0.018) s until 59275 MJD. A recent NuSTAR observation finds the pulse period of the source: (526.2341 0.0041) s. The pulse profile exhibits a transition from double-peaked to single-peaked nature above 30 keV. We analyzed the overall trend of the temporal evolution of fundamental Cyclotron Resonance Scattering Feature (CRSF), , incorporating recent NuSTAR measurements.…
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