Astrophysical Evidence for Black Holes

Abstract

The case for collapsed objects in some X-ray binary systems continues to strengthen. But there is now even firmer evidence for supermassive black holes in galactic centres. Gravitational collapse seems to have occurred in the centres of most newly-forming galaxies, manifesting itself in a phase of quasar-like activity (which may be reactivated later). These phenomena (especially the gas-dynamical aspects) are still a daunting challenge to theorists, but there is `cleaner' evidence, based on stellar dynamics, for collapsed objects in the centres of most nearby galaxies. The current evidence does not tell us the spin of the collapsed objects -- nor, indeed, whether they are described by Kerr geometry, as general relativity theory predicts. There are now, however, several hopeful prospects of discovering observational signatures that will indeed probe the strong-gravity domain.