Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7227
Title: Probing the Cyclotron line characteristics of 4U 1538–522 using AstroSat-LAXPC
Authors: Maitra, Chandreyee
Pradhan, Pragati
Paul, Biswajit
Raichur, Harsha
Varun
Keywords: binaries
general – radiation mechanism
non-thermal – (stars:) pulsars
general – (stars:) pulsars
individual
4U 1538-522 –X-rays
stars
Issue Date: 1-Mar-2019
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2019, Vol. 484, p L1–L6
Abstract: We report the first report on cyclotron line studies with the LAXPC instrument onboard AstroSat of the high-mass X-ray binary pulsar 4U 1538–52. During the observation of source that spanned about 1 d with a net exposure of 50 ks, the source X-ray flux remained constant. Pulse profile is double peaked in low-energy range and has a single peak in high-energy range, the transition taking place around the cyclotron line energy of the source. Cyclotron scattering feature (CRSF) is detected at ∼22 keV with a very high significance in phase-averaged spectrum. It is one of the highest signal to noise ratio detections of CRSF for this source. We performed detailed pulse-phase-resolved spectral analysis with 10 independent phase bins. We report the results of pulse-phase-resolved spectroscopy of the continuum and CRSF parameters. The cyclotron line parameters show pulse phase dependence over the entire phase with a CRSF energy variation of ∼13 per cent⁠, which is in agreement with previous studies. We also confirm the increase in the centroid energy of the CRSF observed between the 1996–2004 (RXTE) and the 2012 (Suzaku) observations, reinforcing that the increase was a long-term change.
Description: Open Access.
URI: http://hdl.handle.net/2289/7227
ISSN: 0035-8711
1365-2966 - (online)
Alternative Location: https://ui.adsabs.harvard.edu/abs/2019MNRAS.484L...1M/abstract
https://arxiv.org/abs/1812.06609
https://doi.org/10.1093/mnrasl/sly234
Copyright: 2019 The Author(s)
Appears in Collections:Research Papers (A&A)

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