http://arxiv.org/abs/2212.10238
The X-ray signal from active galactic nuclei and black hole X-ray binaries is highly variable on a range of timescales. This variability can be exploited to map the region of interest close to the black hole, which is far too small to directly image for all but two black holes in the Universe. Spectral-timing techniques provide causal information by combining timing and spectral information. I present a brief review of such techniques, focusing on two examples: X-ray reverberation mapping and phase-resolved spectroscopy of low frequency quasi-periodic oscillations (LF QPOs). The former provides a means to diagnose the accretion geometry and measure parameters such as black hole mass, and the latter gives perhaps the best constraints we currently have as to the enigmatic LF QPO mechanism.
A. Ingram
Wed, 21 Dec 22
57/81
Comments: Proceeding from the conference “Black Hole Accretion Under the X-ray Microscope” in ESAC, Madrid, 14-17th June 2022. Accepted for publication in Astronomical Notes. 6 pages, 3 figures