Probing the Cyclotron line characteristics of 4U 1538-522 using AstroSat-LAXPC

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 which spanned about one day 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 $\sim$ 22 keV with a very high significance in phase averaged spectrum. It is one of the highest signal to noise ratio detection 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 $\sim$ 13% 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.

6 pages, 7 figures, Accepted for publication in MNRAS Letter

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Cited by in corpus (5)

• The First NuSTAR Observation of 4U 1538-522: Updated Orbital Ephemeris and A Strengthened Case for an Evolving Cyclotron Line Energy
• New measurements of the cyclotron line energy in Cen X-3
• Torque reversal and cyclotron absorption feature in HMXB 4U 1538-522
• Long-term evolution of Cyclotron Line energy in an eclipsing pulsar 4U 1538-522
• Sidebands to mHz QPOs in 4U 1626$-$67 in the second spin-down state