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Papers

Properties of the Binary Neutron Star Merger GW170817

http://dx.doi.org/10.1103/PhysRevX.9.011001

  • AuthorB.P. Abbott et al.,김환선,손재주,오상훈,오정근
  • JournalPhysical Review X (2160-3308), 9(1), 011001-1 ~ 011001-32
  • Enrollment typeSCI
  • publication date 20190102
On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy.