Temporal and spectral study of the X-ray pulsar 2S 1553-542 during the 2021 outburst

Abstract

We study the timing and spectral properties of the X-ray pulsar 2S 1553--542 using the NuSTAR, and NICER during the outburst in January--February 2021. During the outburst, the spin period of the neutron star was 9.2822 s based on NuSTAR data. The pulse profiles are studied using different NICER observations, which implies that the profile is more or less sinusoidal with a single peak and the beaming patterns are mostly dominated by the pencil beam. The NICER spectra of the source are studied for different days of the outburst and can be well described by a model consisting of a blackbody emission and power law along with a photoelectric absorption component. The variation of spectral parameters with luminosity is studied over the outburst. The photon index shows anti-correlation with luminosity below the critical luminosity, which implies that the source was accreting in the sub-critical accretion regime during the NICER observations. We also report the anti-correlation between pulsed fraction (PF) and luminosity of the 2S 1553--542 using NICER observations. The evolution of spin-up rate with luminosity is studied during the outburst, which implies that both are strongly correlated. The torque-luminosity model is applied to estimate the magnetic field at different spin-up rates. The magnetic field is estimated to be 2.56 $\times 10^{12}$ G from the torque-luminosity model using the source distance of 20 kpc. The magnetic field is also estimated using the critical luminosity, which is also consistent with our findings.

Accepted for publication in Journal of Astrophysics and Astronomy

References in corpus (9)

• An Empirical Background Model for the NICER X-ray Timing Instrument
• Decade long RXTE monitoring observations of Be/X-ray binary pulsar EXO 2030+375
• Correlation between the luminosity and spin-period changes during outbursts of 12 Be binary pulsars observed by the MAXI/GSC and the Fermi/GBM
• 2S1553-542: a Be/X-ray binary pulsar on the far side of the Galaxy
• Study of timing and spectral properties of the X-ray pulsar 1A 0535+262 during the giant outburst in 2020 November-December
• Timing and spectral analysis of 2S 1417$-$624 during its 2018 outburst
• Broadband X-ray characteristics of the transient pulsar GRO J2058+42
• Accreting on the edge: a luminosity-dependent cyclotron line in the Be/X-ray Binary 2S 1553-542 accompanied by accretion regimes transition
• Timing and Spectral Studies of the X-ray Pulsar 2S 1417$-$624 During the Outburst in 2021

Cited by in corpus (1)

• Pulse frequency variations and timing noise of MXB 0656-072 during the 2007-2008 type I outbursts and implications for its magnetic field