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We present long slit spectra and multi-color CCD images which demonstratethat the strong star formation episodes that occurred in the post-starburstgalaxies in the Coma Cluster and two field galaxies were not restricted to thecentral regions of the galaxies. Rather, the remnant young stars from thestarbursts are found to be distributed over a large radius, though changes inthe relative strength of the old and young components with radius are evidentin a few cases. The Coma galaxies are shown to have exponential disk profiles,and the spectra provide further kinematical evidence that the galaxies arerotating systems, indicating that the galaxies are not ellipticals. Thestarburst material also appears to be distributed in disks. Such informationplaces constraints on models for the starbursts that involve mergers. Someemission line galaxies are also discussed.Comment: 22 pages + 13 of 15 figures, uuencoded gzipped postscript. Text and  Figs 9 and 10 also available at ftp://flwo99.sao.arizona.edu To appear in  Jan. A

Spatial Distribution of the Starbursts in Post-Starburst Coma Cluster Galaxies