Radial-dependent Responsivity of Broad-line Regions in Active Galactic Nuclei: Observational Consequences for Reverberation Mapping and Black Hole Mass Measurements

TL;DR

This paper develops a unified theoretical framework for reverberation mapping of active galactic nuclei, incorporating radial-dependent responsivity of broad-line regions to improve black hole mass measurements.

Contribution

It introduces a rigorous, analytically expressed model for BLR responsivity and transfer functions, accounting for radial dependence and continuum variability effects.

Findings

RMS spectra are biased unless continuum variation timescale is long.

Radial-increasing responsivity explains differences between mean and RMS spectra.

Virial factors depend on luminosity states, not just geometry and kinematics.

Abstract

The reverberation mapping (RM) technique has seen wide applications in probing geometry and kinematics of broad-line regions (BLRs) and measuring masses of supermassive black holes (SMBHs) in active galactic nuclei. However, the key quantities in RM analysis like emissivity, responsivity, transfer functions, and mean and root-mean-square (RMS) spectra are fragmentally defined in the literature and largely lack a unified formulation. Here, we establish a rigorous framework for BLR RM and include a locally dependent responsivity according to photoionization calculations. The mean and RMS spectra are analytically expressed with emissivity- and responsivity-weighted transfer functions, respectively. We demonstrate that the RMS spectrum is proportional to the responsivity-weighted transfer function only when the continuum variation timescale is much longer than the typical extension in time delay of the BLR, otherwise, biases arise in the obtained RMS line widths. The long-standing phenomenon as to the different shapes between mean and RMS spectra can be explained by a radial-increasing responsivity of BLRs. The debate on the choice of emission line widths for SMBH mass measurements is explored and the virial factors are suggested to also depend on the luminosity states, in addition to the geometry and kinematics of BLRs.