Infrared Interferometry of the active galaxy NGC 1068
Research report (imported) 2004 - Max Planck Institute for Radio Astronomy
Summary
Speckle-interferometric observations as well as long-baseline interferometry with the instruments VINCI and MIDI at the Very Large Telescope Interferometer (VLTI) have allowed the resolution of the nucleus of the Active Galaxy NGC 1068 at infrared wavelengths in the range of 1,65 to 13 µm. Therefore, it is now possible, for the first time, to investigate the inner torus region around NGC 1068’s Black Hole and to test model predictions.