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We present Herschel-SPIRE observations at 250-500um of the giant ellipticalgalaxy M86 and examine the distribution of the resolved cold dust emission andits relation with other galactic tracers. The SPIRE images reveal three dustcomponents: emission from the central region; a dust lane extendingnorth-south; and a bright emission feature 10kpc to the south-east. We estimatethat approximately 10^6 solar masses of dust is spatially coincident withatomic and ionized hydrogen, originating from stripped material from the nearbyspiral NGC4438 due to recent tidal interactions with M86. The gas-to-dust ratioof the cold gas component ranges from ~20-80. We discuss the different heatingmechanisms for the dust features.

The dust morphology of the elliptical Galaxy M86 with SPIRE