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Constraining the progenitors of short gamma ray bursts

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Figure

Figure 1.1: BATSEels show GRBs which display a single peak: on the left is a (short) GRB with a fast-rise, exponential decay (FRED) profile and on the right a simple peak
Figure 1.2: T90 vs Hardness Ratio for BATSE (grey starred points) and Swift (red trian-gles)
Figure 1.4: Evolution of two main sequence stars of differing initial masses:and 8star evolves off the main sequence first filling its Roche lobe
Figure 1.6: The synchrotron emission from shocked electrons in the ultra-relativistic jetswhich the electrons lose significant energy from radiation
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