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Long-duration ($>2$ s) $\gamma$-ray bursts that are believed to originate from the death of massive stars are expected to be accompanied by supernovae.
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D. Grossman, O. Korobkin, S. Rosswog, and T. Piran. The long-term evolution of neutron star merger remnants - II. Radioactively powered transients · 2014
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O. Korobkin, S. Rosswog, A. Arcones, and C. Winteler. On the astrophysical robustness of the neutron star merger r-process · 2012
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E. Berger, W. Fong, and R. Chornock. An r-process Kilonova Associated with the Short-hard GRB 130603B · 2013
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M. Tanaka, and K. Hotokezaka. Radiative Transfer Simulations of Neutron Star Merger Ejecta · 2013
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2015
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O. Just, A. Bauswein, R. A. Pulpillo, S. Goriely, and H. T. Janka. Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers · 2015
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R. Fernández, E. Quataert, J. Schwab, D. Kasen, and S. Rosswog. The interplay of disk wind and dynamical ejecta in the aftermath of neutron star - black hole mergers · 2015
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