paper

Detection of X-ray/UV delay in NGC 4051 using AstroSat observations

arXiv:2311.02722 · doi:10.1093/mnras/stad3444

Abstract

We study the connection between the variations in the far ultra-violet (FUV), near ultra-violet (NUV) and X-ray band emission from NGC 4051 using 4-days long AstroSat observations performed during 5-9 June 2016. NGC 4051 showed rapid variability in all three bands with the strongest variability amplitude in the X-ray band () and much weaker variability in the UV bands (). Cross-correlation analysis performed using Interpolated cross-correlation Functions (ICCF) and Discrete cross-correlation Functions (DCF) revealed a robust correlation () between the UV and X-ray light curves. The variations in the X-ray band are found to lead those in the FUV and NUV bands by and , respectively. The UV lags favour the thermal disc reprocessing model. The FUV and NUV bands are strongly correlated () and the variations in the FUV band lead those in the NUV band by . Comparison of the UV lags found using the AstroSat observations with those reported earlier and the theoretical model for thermal reverberation time-lag suggests a possible change in either the geometry of the accretion disc/corona or the height of the corona.

8 pages, 5 figures, Accepted for publication in MNRAS

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