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A kilonova following a long-duration gamma-ray burst at 350 Mpc - Nature

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A kilonova following a long-duration gamma-ray burst at 350 Mpc - Nature

Gamma-ray bursts (GRBs) are divided into two populations1,2; long GRBs that derive from the core collapse of massive stars (for example, ref. 3) and short GRBs that form in the merger of two compact objects4,5. Although it is common to divide the two populations at a gamma-ray duration of 2 s, classification based on duration does not always map to the progenitor.

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A kilonova following a long-duration gamma-ray burst at 350 Mpc - Nature

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A kilonova following a long-duration gamma-ray burst at 350 Mpc - Nature

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