Abstract Details

Name: Jithesh V
Affiliation: IUCAA, Pune
Conference ID: ASI2020_159
Title : AstroSat View of the new Galactic X-Ray Transient Swift J1658.2-4242
Authors and Co-Authors : V. Jithesh, Bari Maqbool, Ranjeev Misra, Athul. R. T, Gitika Mall and Marykutty James
Abstract Type : Poster
Abstract Category : Stars, ISM and Galaxy
Abstract : We present the X-ray timing and spectral analysis of the new Galactic X-ray transient Swift J1658.2-4242 observed with LAXPC and SXT instruments onboard AstroSat. We detect prominent C-type quasi-periodic oscillations (QPOs) of frequencies varying from ~ 1.5 Hz to ~ 6.6 Hz along with distinct 2nd harmonics and sub-harmonics. The QPO detected at ~ 1.56 Hz drifts to a higher centroid frequency of ~ 1.74 in the course of the observation, while the QPO detected at ~ 6.6 Hz disappeared during hard flarings. The fractional rms at the QPO and the sub-harmonic frequencies increases with photon energy, while at the 2nd harmonic frequencies the rms seems to be constant. In addition, we have observed soft time lag at QPO and sub-harmonic frequencies up to a time scale of ~ 35 ms, however, at the 2nd harmonic frequencies there is weak/zero time lag. We attempt spectral modeling of the broadband data in the 0.7–25 keV band using the doubly absorbed disk plus thermal Comptonization model. Based on the spectral and timing properties, we identified the source to be in the hard intermediate state of black hole X-ray binaries. To quantitatively fit the energy and frequency-dependent fractional rms and time lag, we use a single zone fluctuation propagation model and discuss our results in the context of that model.