Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993 - The Dark Energy Survey

Evidence for Dynamically Driven Formation of the GW170817 Neutron Star Binary in NGC 4993

October 18, 2017 | Antonella Palmese et al.

« THE ELECTROMAGNETIC COUNTERPART OF THE BINARY NEUTRON STAR MERGER LIGO/VIRGO GW170817. I. DISCOVERY OF THE OPTICAL COUNTERPART USING THE DARK ENERGY CAMERA

Photometric characterization of the Dark Energy Camera »