On Nulling Interferometers and the Line-Emitting Regions of AGNs

Abstract

The nulling interferometers proposed to study planets around other stars are generally well suited for studying small-scale structures surrounding other bright pointlike objects such as the nuclei of active galaxies. Conventional interferometric techniques will produce useful maps of optical/IR line and continuum emission within active galaxies on scales of 10 milliarcseconds (mas), but similar studies of broad-line regions will require baselines longer than those currently envisaged. Nevertheless, nulling interferometers currently under development will be able to constrain quasar velocity fields on milliarcsecond scales, as long as they are equipped with spectrographs capable of resolving lines several hundred km/s wide. This Letter describes how analyses of line emission leaking through the edges of the null in such an instrument can reveal the size, shape, and velocity field of nebular gas on the outskirts of a quasar broad-line region. If this technique proves effective, it could potentially be used to measure the mass function of quasar black holes throughout the universe.