The Nuclear Star Cluster and Central Massive Black Hole


Reinhard Genzel

Max Planck Institute for Extraterrestrial Physics Garching Germany
& Professor of Physics, University of California, Berkeley

Abstract

In the past decade high resolution measurements in the infrared
employing adaptive optics imaging on 10m telescopes have allowed
determining the three dimensional orbits stars within ten light hours
of the compact radio source SgrA* at the Center of the Milky Way.
These observations show that SgrA* is a three million solar mass black
hole, beyond any reasonable doubt. The Galactic Center thus
constitutes the best astrophysical evidence for the existence of black
holes which have long been postulated, and is also an ideal 'lab' for
studying the physics in the vicinity of such an object. Remarkably,
young massive stars are present there and probably have formed in the
innermost stellar cusp. Variable infrared and X-ray emission from SgrA*
are a new probe of the physics and space time just outside the event
horizon.