  The background field of the Tadpole galaxy image taken with the Hubble Space
Telescope ACS contains 87 clump-clusters that are probably low-inclination
versions of the 69 chain galaxies we found in a previous paper. This conclusion
follows from the similarity in colors and apparent magnitudes of the brightest
clumps in the clump-clusters and chain galaxies, and from the similarity
between the distribution of axial ratios for the combined sample and the
distribution for normal disk galaxies. These distributions are consistent with
chains and clump-clusters being disks viewed at random angles with intrinsic
axial ratios of 0.1-0.2 or less. The disks appear to be gas-rich galaxies at
z=1 to 2 that are forming an early generation of stars in a small number of
very large star complexes.
