Mid-Infrared observations of NGC 1068 with ISOCAM

We report on Mid-Infrared (MIR) observations of the Seyfert 2 galaxy NGC 1068, obtained with ISOCAM in low-resolution spectro-imaging mode. The spatial resolution of the data (~ 6″) allows us to disentangle the circumnuclear starburst regions from the emission of the active galactic nucleus (AGN).