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The Macronova in GRB 050709 and the GRB-macronova connection.


ABSTRACT: GRB 050709 was the first short Gamma-ray Burst (sGRB) with an identified optical counterpart. Here we report a reanalysis of the publicly available data of this event and the discovery of a Li-Paczynski macronova/kilonova that dominates the optical/infrared signal at t>2.5 days. Such a signal would arise from 0.05 r-process material launched by a compact binary merger. The implied mass ejection supports the suggestion that compact binary mergers are significant and possibly main sites of heavy r-process nucleosynthesis. Furthermore, we have reanalysed all afterglow data from nearby short and hybrid GRBs (shGRBs). A statistical study of shGRB/macronova connection reveals that macronova may have taken place in all these GRBs, although the fraction as low as 0.18 cannot be ruled out. The identification of two of the three macronova candidates in the I-band implies a more promising detection prospect for ground-based surveys.

SUBMITTER: Jin ZP 

PROVIDER: S-EPMC5036160 | biostudies-literature | 2016 Sep

REPOSITORIES: biostudies-literature

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The Macronova in GRB 050709 and the GRB-macronova connection.

Jin Zhi-Ping ZP   Hotokezaka Kenta K   Li Xiang X   Tanaka Masaomi M   D'Avanzo Paolo P   Fan Yi-Zhong YZ   Covino Stefano S   Wei Da-Ming DM   Piran Tsvi T  

Nature communications 20160923


GRB 050709 was the first short Gamma-ray Burst (sGRB) with an identified optical counterpart. Here we report a reanalysis of the publicly available data of this event and the discovery of a Li-Paczynski macronova/kilonova that dominates the optical/infrared signal at t>2.5 days. Such a signal would arise from 0.05 r-process material launched by a compact binary merger. The implied mass ejection supports the suggestion that compact binary mergers are significant and possibly main sites of heavy r  ...[more]

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