We propose to make sensitive, spatially-resolved observations of the
 region around the unusual intergalactic HI cloud lying between the
 giant elliptical, NGC4472, and the dwarf irregular, UGC7636 with
 ISO PHT-C at 120 and 200 microns.  Recent optical and radio
 observations suggest that this cloud has been ram-pressure-stripped
 by the hot, dense, X-ray halo of NGC4472 from the tidally-distorted
 tail of the dwarf.  There appears to be little star-formation in the
 disturbed region.  These observations will look for cool dust
 spatially co-extensive with the HI cloud.  If cool dust is detected,
 this will add further support for the hypothesis that some dwarf
 elliptical galaxies are formed by stripping of gas from dwarf
 irregular systems.  These observations will also allow us to set
 limits on star formation in the HI cloud system. The physical
 conditions in dwarf galaxies, which are similar, are poorly
 understood. ISO observations may allow us to catch the evolution
 of an unique, transitory object at an early stage.