  We present long slit spectra and multi-color CCD images which demonstrate
that the strong star formation episodes that occurred in the post-starburst
galaxies in the Coma Cluster and two field galaxies were not restricted to the
central regions of the galaxies. Rather, the remnant young stars from the
starbursts are found to be distributed over a large radius, though changes in
the relative strength of the old and young components with radius are evident
in a few cases. The Coma galaxies are shown to have exponential disk profiles,
and the spectra provide further kinematical evidence that the galaxies are
rotating systems, indicating that the galaxies are not ellipticals. The
starburst material also appears to be distributed in disks. Such information
places constraints on models for the starbursts that involve mergers. Some
emission line galaxies are also discussed.
