COMPTEL GAMMA-RAY BURST OBSERVATIONS
                              
   R.M. Kippen, A. Connors, D. Forrest, M. McConnell,
   J. Ryan, (UNH), W. Collmar, R. Diehl, V.
   Schšnfelder, H. Steinle, M. Varendorff (MPE), J.W.
   den Herder, W. Hermsen, L. Kuiper, B.N. Swanenburg,
   C. de Vries (ROL), K. Bennett, L. Hanlon, O.R.
   Williams, C. Winkler (SSD/ESA)
   
   The  COMPTEL  experiment on  the  Compton  Gamma  Ray
   Observatory   regularly  observes  gamma-ray   bursts
   occurring within its 1 steradian field of  view.   In
   its  primary telescope mode of operation, COMPTEL has
   the  ability to directly image 0.75-30 MeV gamma-rays
   from   these  sources  yielding  locations  with   an
   accuracy of about 1 degree.  Spectral information  is
   acquired   in  the  telescope  mode  with  resolution
   better  than 10% FWHM.  During transient events  such
   as  gamma-ray  bursts, time-resolved  energy  spectra
   are  also recorded from COMPTEL's individual D2 (NaI)
   burst  detectors (0.1-10 MeV).  This  paper  presents
   recent  results  on  gamma-ray  bursts  observed   by
   COMPTEL.
   
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