Occultation mapping of the central engine in the active galaxy MCG -6-30-15

The colossal power output of active galactic nuclei (AGNs) is believed to be fueled by the accretion of matter onto a supermassive black hole. This central accreting region of AGNs has hitherto been spatially unresolved, and its structure therefore unknown. Here we propose that a previously reported "deep minimum" in the X-ray intensity of the AGN MCG -6-30-15 was due to a unique X-ray occultation event and that it probes structure of the central engine on scales smaller than 10(14) crn, or 1.4 x 10(-7) arcsec. This resolution is more than a factor of similar to 3 x 10(6) greater than is possible with current X-ray optics. The data are consistent with a bright central sourer surrounded by a less intense ring, which we identify with the inner edge of an accretion disk. These may be the first direct measurements of the spatial structure and geometry of the accreting black hole system in an active galaxy. We estimate a mass lower limit for sub-Eddington accretion of 3.1 x 10(5) M-.. If the ring of Xray emission is identified with the inner edge of an accretion disk, we get mass upper limits of 1.9 x 10(8) and 9.1 x 10(8) M-. for a nonrotating and maximally rotating black hole, respectively. We point out that our occultation interpretation is controversial in the sense that X-ray variability in AGNs is normally attributed to intrinsic physical changes in the X-ray emission region, such as disk or coronal instabilities.