Ackermann, M.M.AckermannAsano, K.K.AsanoAtwood, W. B.W. B.AtwoodTosti, G.G.TostiGasparrini, DarioDarioGasparrini2020-09-172020-09-172010-06-01https://hdl.handle.net/20.500.13025/1785The Astrophysical Journal, Volume 716, Issue 2, pp. 1178-1190 (2010).We present detailed observations of the bright short-hard gamma-ray burst GRB 090510 made with the Gamma-ray Burst Monitor (GBM) and Large Area Telescope (LAT) on board the Fermi observatory. GRB 090510 is the first burst detected by the LAT that shows strong evidence for a deviation from a Band spectral fitting function during the prompt emission phase. The time-integrated spectrum is fit by the sum of a Band function with E <SUB>peak</SUB> = 3.9 0.3 MeV, which is the highest yet measured, and a hard power-law component with photon index -1.62 0.03 that dominates the emission below &ap;20 keV and above &ap;100 MeV. The onset of the high-energy spectral component appears to be delayed by ~0.1 s with respect to the onset of a component well fit with a single Band function. A faint GBM pulse and a LAT photon are detected 0.5 s before the main pulse. During the prompt phase, the LAT detected a photon with energy 30.5<SUP>+5.8</SUP> <SUB>-2.6</SUB> GeV, the highest ever measured from a short GRB. Observation of this photon sets a minimum bulk outflow Lorentz factor, Gammagsim 1200, using simple gammagamma opacity arguments for this GRB at redshift z = 0.903 and a variability timescale on the order of tens of ms for the &ap;100 keV-few MeV flux. Stricter high confidence estimates imply Gamma >~ 1000 and still require that the outflows powering short GRBs are at least as highly relativistic as those of long-duration GRBs. Implications of the temporal behavior and power-law shape of the additional component on synchrotron/synchrotron self-Compton, external-shock synchrotron, and hadronic models are considered.gamma-ray burst individual GRB 090510radiation mechanisms non-thermal10.1088/0004-637X/716/2/1178http://adsabs.harvard.edu/abs/2010ApJ...716.1178A2010ApJ...716.1178A