General relativistic magnetohydrodynamic simulations of binary neutron star mergers forming a long-lived neutron star
R. Ciolfi(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), Rosalba Perna(Stony Brook University)
Cited by 182
Related Papers
Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger
|Nature|2017|981
The THESEUS space mission concept: science case, design and expected performances
|Advances in Space Research|2018|208
The optical afterglows and host galaxies of three short/hard gamma-ray bursts
|Astronomy and Astrophysics|2009|87
THESEUS: A key space mission concept for Multi-Messenger Astrophysics
|Advances in Space Research|2018|86
A comparison between short GRB afterglows and kilonova AT2017gfo: shedding light on kilonovae properties
|Monthly Notices of the Royal Astronomical Society|2020|85