17th Texas Symposium on Relativistic Astrophysics ------------------------------------------------- COMPTEL OBSERVATIONS OF GAMMA-RAY BURSTS R.M. Kippen, A. Connors, M. McConnell, J. Ryan (University of New Hampshire) W. Collmar, J. Greiner, V. Schoenfelder, M. Varendorff (Max-Planck Institut fur Extraterrische Physik) W. Hermsen, L. Kuiper (SRON-Utrecht) L.O. Hanlon, K.S. O'Flaherty, C. Winkler (Astrophysics Division, ESTEC) The Imaging Compton Telescope (COMPTEL) onboard the Compton Gamma Ray Observatory regularly detects cosmic gamma-ray bursts. Energy spectra and temporal profiles are obtained both from the main instrument (0.75-30 MeV) and independent burst modules (0.1-10 MeV). Analysis of these measurements indicate a wide variety of different temporal structures and energy spectra which are in most cases well- described by a single power-law model with spectral index ~2-3. Several of these events show evidence of significant spectral evolution. In its first three years of operation, 18 significant bursts occurring within the ~1 sr field-of-view of the main instrument have been localized through direct imaging with an average accuracy of ~1 deg. The locations of these bursts are consistent with an isotropic distribution of sources, however two of the events coincide spatially well within the instrumental errors. The probability of such a coincidence occurring by chance in an isotropic distribution has been estimated to be ~3% -- suggesting the possibility that these two events are somehow related to a single source. Several of the COMPTEL bursts were localized within hours of their occurrence, initiating world-wide multiwavelength searches for fading counterpart emission in record time. No obvious counterparts have yet been identified, however COMPTEL observes new bursts at a rate of ~1/month and the localization response-time continues to improve. We present an overview of COMPTEL gamma-ray burst results and an update on new observations, including rapidly imaged events. -eof-