WFPC2 images can be combined with complementary observations in other wavelength regimes to identify cloudlets inside remnants, trace SNR shock fronts, determine the physical parameters of interior cloudlets and compare them to those of the hot interior, and investigate the evaporation of shocked cloudlets into the hot cavities of the SNRs. This survey will be useful to study the star formation histories, chemical evolution, and distances to these galaxies. These data will be placed immediately into the Hubble Data Archive. The observations were completed as scheduled, and no problems were reported. Otherwise, the observations completed with no further anomalous activity.
Uncertainty is caused by the fact that a zone of exclusion was involved.
Proposals described in 1.13 and 1.15 were affected. Continuation of normal science observations and calibrations.