Spectro-temporal investigation of the black hole X-ray transient 4U 1543-475 during the 2021 outburst
Biki Ram, Manoneeta Chakraborty, Unnati Kashyap

TL;DR
This study provides a detailed spectro-temporal analysis of the 2021 outburst of black hole binary 4U 1543-475, revealing state transitions, variability components, and disk-corona interactions through AstroSat observations.
Contribution
It offers new insights into the variability evolution and flip-flop phenomena in black hole X-ray binaries during outbursts, emphasizing the roles of disk and coronal changes.
Findings
Emergence of band-limited noise during state transition
Correlation between low-frequency variability and non-thermal component
Detection of flip-flop phenomenon with rapid flux and RMS variation
Abstract
We report a detailed spectro-temporal analysis of the black hole (BH) low mass X-ray binary (LMXB) 4U 1543-475 during its 2021 outburst using the data from LAXPC (Large Area X-ray Proportional Counters) and SXT (Soft X-ray Telescope) instrument on board AstroSat. We investigate the energy and frequency dependency of the source variability to probe the origin of the disc/coronal fluctuations. Following the state transition (from soft to intermediate state), the emergence of a band-limited noise (BLN) component is observed along with the power law noise (PLN) when the disk is recovering from a sudden decrease in the inner disk radius. A possible correlation between the low-frequency variability amplitude (RMS) and the covering fraction of the non-thermal component is detected. During the final AstroSat observation, a flip-flop phenomenon is reported, where rapid variation in RMS occurs in…
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Taxonomy
TopicsAstrophysical Phenomena and Observations
