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Late time afterglow observations reveal a collimated relativistic jet in the ejecta of the binary neutron star merger GW170817
Davide Lazzati, Rosalba Perna, Brian J. Morsony +5
The binary neutron star (BNS) merger GW170817 was the first astrophysical source detected in gravitational waves and multi-wavelength electromagnetic radiation. The almost simultan…
Prompt Electromagnetic Transients from Binary Black Hole Mergers
Bernard J. Kelly, John G. Baker, Zachariah B. Etienne +2
Binary black hole (BBH) mergers provide a prime source for current and future interferometric GW observatories. Massive BBH mergers may often take place in plasma-rich environments…
The Fate of Neutron Star Binary Mergers
Anthony L. Piro, Bruno Giacomazzo, Rosalba Perna
Following merger, a neutron star (NS) binary can produce roughly one of three different outcomes: (1) a stable NS, (2) a black hole (BH), or (3) a supra-massive, rotationally-suppo…
General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
Riccardo Ciolfi, Wolfgang Kastaun, Bruno Giacomazzo +3
Merging binary neutron stars (BNSs) represent the ultimate targets for multimessenger astronomy, being among the most promising sources of gravitational waves (GWs), and, at the sa…