http://arxiv.org/abs/1706.02316
The X-ray emitting corona irradiates and ionises the surface of the inner accretion disc in Active Galactic Nuclei (AGNs). The ionisation parameter of the inner disc at a radius $r$ from the black hole, $\xi(r)$, can be used to infer information about the location of the corona. Here, a new formula is derived that predicts $\xi(r,h)$ for a disc irradiated by a X-ray source at a height $h$ above the black hole symmetry axis (i.e., a lamppost geometry). The equation is independent of the black hole mass and the X-ray spectrum, and accounts for the effects of gravitational light-bending on the ionisation state and a variable coronal dissipation factor. We predict a strong ionisation gradient across the surface of the inner disc that depends on the black hole spin and lamppost height. For a fixed $h$, the ionisation parameter is also expected to increase as $\lambda^3$, where $\lambda$ is the observed bolometric Eddington ratio of the AGN. Comparing this formula to the observed $\xi$-$\lambda$ relationship for Mrk 335 yields $h \propto \lambda^{0.5-0.6}$, supporting the view of a dynamic X-ray corona in AGNs.
D. Ballantyne
Fri, 9 Jun 17
37/52
Comments: 5 pages, 5 figures, submitted to MNRAS Letters
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