A Reverse Shock In GRB 160509A

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Long duration γ-ray bursts (GRBs) are produced during the catastrophic collapse of massive stars (MacFadyen & Woos- ley 1999), their immense luminosity likely powered by relativistic outflows launched from a compact central engine(Piran 2005). However, the nature of the central engine launching the outflow and the mechanism producing the collimated, relativistic jet remain two urgent open questions,
with models ranging from jets dominated by baryons or by Poynting flux, and those with nascent black holes or magnetars providing the central engine (see Kumar & Zhang 2015, for a review).

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