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Improved data analysis of far infrared imaging data of the globular cluster NGC 7078 obtained with the ISO instru- ment ISOPHOT at 60 µm, 70 µm and 90 µm has detected the thermal emission from dust in its core, the first secure detection of intra-cluster dust in a globular cluster. The amount of dust is broadly consistent with mass-loss from evolved, metal-deficient stars in NGC 7078 in the time since it last crossed the Galactic plane.

Far infra-red emission from NGC 7078: First detection of intra-cluster dust in a globular cluster