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Supernova and Prompt Gravitational-wave Precursors to LIGO Gravitational-wave Sources and Short GRBs
2018
Astrophysical Journal Letters
Binary black-holes (BHs) and binary neutron-stars (NSs) mergers had been recently detected through gravitational-wave (GW) emission, with the latter followed by post-merger electromagnetic counterparts, appearing seconds up to weeks after the merger. While post-merger electromagnetic counterparts had been anticipated theoretically, very little electromagnetic precursors to GW-sources had been proposed, and non observed yet. Here we show that a fraction of a few×10^-4-10^-1 of LIGO GW-sources
doi:10.3847/2041-8213/aaacfc
fatcat:c4ttna53mrh6hewcf4wploef6y