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Session 11 - AGN.
Display session, Monday, January 13
ISOCAM maps of the Seyfert 1 S0 galaxy NGC 3998 between 4.5\rm\mu m and 15\rm\mu m detect both extended emission from the bulge stars and strong point source emission from the nucleus. The inner regions of NGC 3998 appear to contain a few thousand solar masses of warm (\sim 200\, K) dust, probably associated with the AGN.
Program listing for Monday