Model comparison from LIGO–Virgo data on GW170817’s binary components and consequences for the merger remnant
© 2020 IOP Publishing Ltd. GW170817 is the very first observation of gravitational waves originating from the coalescence of two compact objects in the mass range of neutron stars, accompanied by electromagnetic counterparts, and offers an opportunity to directly probe the internal structure of neut...
Main Authors: | LIGO Scientific Collaboration, Virgo Collaboration |
---|---|
Other Authors: | LIGO (Observatory : Massachusetts Institute of Technology) |
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2021
|
Online Access: | https://hdl.handle.net/1721.1/132423 |
Similar Items
-
GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
by: LIGO Scientific Collaboration, et al.
Published: (2018) -
Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817
by: LIGO Scientific Collaboration, et al.
Published: (2018) -
On the Progenitor of Binary Neutron Star Merger GW170817
by: LIGO Scientific Collaboration, et al.
Published: (2018) -
Properties and Astrophysical Implications of the 150 M ⊙ Binary Black Hole Merger GW190521
by: LIGO Scientific Collaboration, et al.
Published: (2021) -
Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1
by: LIGO Scientific Collaboration, et al.
Published: (2021)