AstroSat detection of a mHz QPO and cyclotron line in IGR J19294+1816 during the 2019 outburst

TL;DR

This paper reports the detection of a mHz QPO and a cyclotron line in the X-ray pulsar IGR J19294+1816 during its 2019 outburst, providing insights into its timing and spectral properties.

Contribution

The study presents the first detection of both a QPO and a cyclotron line in IGR J19294+1816 during an outburst, highlighting its complex spectral and timing features.

Findings

Detected a QPO at 0.032 Hz with 18% RMS amplitude.

Measured a cyclotron line at 42.7 keV.

Determined a spin period of 12.485 s.

Abstract

We present results from timing and spectral analysis of the HMXB X-ray pulsar IGR J19294+1816 observed using \asr during its recent Type-I outburst in October, 2019. AstroSat observations sampled the outburst at the decline phase right after the outburst peak. We carried out timing analysis on the light curves obtained using the Large Area X-ray Proportional Counter (LAXPC) instrument on board AstroSat and measured a spin period of 12.485065$\pm$0.000015 s. The peak in the power density spectrum (PDS) corresponding to the spin period of 12.48 s also shows a broadened base. We also detected a Quasi Periodic Oscillation (QPO) feature at 0.032$\pm$0.002 Hz with an RMS fractional amplitude of $\sim$18% in the PDS. We further carried out a joint spectral analysis using both the Soft X-ray Telescope (SXT) and the LAXPC instruments and detected a Cyclotron Resonant Scattering Feature (CRSF) at 42.7$\pm$0.9 keV and an Fe emission line at 6.4$\pm$0.1 keV. IGR J19294+1816, being an intermediate spin pulsar, has exhibited a plethora of spectral and timing features during its most recent 2019 outburst, adding it to the list of transients that exhibit both a QPO as well as a CRSF.