Investigating the Periodic X-Ray Behaviour in the Eclipsing AGN NGC 6814

Le résumé fourni par la source

Abstract A 2016 XMM-Newton X-ray light curve of the Seyfert 1.5 galaxy NGC 6814 exhibited clear eclipsing behavior, with distinct ingress and egress, during half of the observation. Here, we report on the periodic behavior in the light curve prior to the eclipse. We use timing and spectral analysis techniques to quantify the behavior and examine the characteristics of the periodic signal. A superlet transform of the X-ray light curve reveals a frequency of ∼45–50 μ Hz in the initial 60 ks of the observation with a detection significance at the >90% level in both the broad (0.3–10 keV) and soft (0.3–1.0 keV) bands. The period is confirmed by fitting a sinusoid, and is also evident in the highest energy bands with diminished significance because of reduced signal-to-noise ratio. There appear to be distinct changes in the variability behavior during the eclipse as the measured period is modulated (stretched) at all energies. From phase-resolved spectra, we investigate possible physical causes of this periodic behavior and find that it can be interpreted as changes in the covering fraction or a nonstandard inner accretion flow (e.g., truncated disk and misaligned flow). The nonstandard inner flow appears consistent with previous reports of a truncated inner disk and compact corona in NGC 6814.

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