The galactic center contains a high concentration of stars and a massive black hole. It also is shrouded in dust that obscures our visual observation of the individual stars. We know there is a black hole there by the intense X-ray and radio emissions that are observable in the constellation Sagittarius, which frames our view of the center of the Milky Way galaxy. The object that is specifically associated with the black hole is Sagittarius A*. To pierce the veil of dust that hides the stars at the center we need to look beyond the visual into other parts of the electromagnetic spectrum—the infrared region.
Looking at the longer wavelengths in the infrared region of the spectrum gives us a view of the heat signature of the stars, which passes through the dust while the visual wavelengths are absorbed by the dust. Looking in the right part of the spectrum is not all you need. You will need an optical system that can resolve, or separately image the individual stars at the center and that takes some special technology, namely adaptive optics and speckle imaging.
Both of these tools are used to compensate for the turbulence we have in our atmosphere due to temperature, pressure and moisture changes. The adaptive optics system adjusts the surface of the mirror of the telescope many times a second after measuring the atmospheric distortion and calculating the best mirror shape to compensate for it. The speckle imaging technique takes many short exposure images, on the order of hundreds to thousands of pictures and then uses a computer and a mathematical algorithm to combine the images to provide a much sharper image.
Utilizing these two advances in technology a team of astronomers lead by Dr. Reinhard Genzel at the Max Planck Institute was able to image the stars at the galactic center over a period of six years, from 1994 to 2000. They produced an amazing movie that shows the stars moving in different orbits about a central mass. The gallery below contains three images taken over this time span that clearly show the motion of the stars. Look closely at the stars in the center of the images and you will see that the pattern changes from frame to frame.