SWIFT view of the 2015 outburst of GS 2023+338 (V404 Cyg): complex evolution of spectral and temporal characteristics
Radhika D., A. Nandi, V. K. Agrawal, S. Mandal

TL;DR
This study provides a detailed analysis of the spectral and temporal evolution of V404 Cyg during its 2015 outburst using SWIFT data, revealing complex state transitions, jet ejections, and wind features.
Contribution
It offers the first comprehensive spectral and temporal analysis of V404 Cyg's 2015 outburst based on SWIFT observations, highlighting unique evolution patterns.
Findings
Source exhibited hard, intermediate, and soft spectral states.
Spectral and temporal evolution differed from typical black hole outbursts.
Wind emission and variable Fe line features suggest outflows and winds.
Abstract
We study the spectral and temporal characteristics of the source GS 2023338 (V404 Cyg) during the initial phase of its June 2015 outburst, over the energy range of 0.5 - 150 keV. This is the first detailed study of the characteristics of this source based on {\it SWIFT} observations, being reported. Based on our analysis, we understand that the source existed in the hard, intermediate and soft spectral states. We find that the evolution of the spectral parameters, the hardness intensity diagram and the rms-intensity diagram are not similar to those observed for most of the outbursting black hole sources. We also observe presence of weak peaked components in the power density spectra during the intermediate state of the source. Dramatic changes in the spectral and temporal properties are also exhibited before the ejection of a radio jet suggesting it to be associated with the coronal…
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