On the Progenitor of Binary Neutron Star Merger GW170817
On 2017 August 17 the merger of two compact objects with masses consistent with two neutron stars was discovered through gravitational-wave (GW170817), gamma-ray (GRB 170817A), and optical (SSS17a/AT 2017gfo) observations. The optical source was associated with the early-type galaxy NGC 4993 at a di...
Similar Items
-
Tests of General Relativity with GW170817
by: LIGO Scientific Collaboration, et al.
Published: (2022) -
GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
by: LIGO Scientific Collaboration, et al.
Published: (2018) -
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
by: LIGO Scientific Collaboration, et al.
Published: (2018) -
Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant
by: LIGO Scientific Collaboration, et al.
Published: (2021) -
Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817
by: LIGO Scientific Collaboration, et al.
Published: (2018)