Images at 24, 70, and 160 μm (from left to right) of the mini-clusters associated with CCDM J2137+5734 (top), 11-2031 (middle), and 213911452+572425205 (bottom). Cluster members (with and without disks) are marked as small cyan stars. Yellow contours at variable levels for each wavelength are shown to mark the structure of the mini-cluster. For the cluster associated with CCDM J2137+5734, whose nebular structure is not detected at Herschel wavelengths, we also overplot the 24 μm contours in cyan in the PACS maps to mark the location of the warm dust.