Figure 1 from The Inner Accretion Flow in the Resurgent Seyfert-1.2 AGN Mrk 817

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Inner Accretion Flow in the Resurgent Seyfert-1.2 AGN Mrk 817

Authors: J. M. Miller, A. Zoghbi, M. T. Reynolds, J. Raymond, D. Barret, E. Behar, W. N. Brandt, L. Brenneman, P. Draghis, E. Kammoun, M. J. Koss, A. Lohfink, and D. K. Stern

2021 The Astrophysical Journal Letters 911 L12.

Provider: AAS Journals

Caption: Figure 1.

The NuSTAR FPMA (black) and FPMB (red) light curves of Mrk 817. The full 3–79 keV count rate is plotted versus time; the time bins are 100 s. Apparent flares or dips are simply edge effects from good time intervals. The overall count rate shows only the “flickering” typical of accreting sources, and no clear trends.

Other Images in This Article

Copyright and Terms & Conditions