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Model comparison from LIGO_Virgo data on GW170817\'s binary components and consequences for the merger remnant

http://10.1088/1361-6382/ab5f7c

  • AuthorB. P. Abbott,김환선,손재주,오상훈,오정근
  • JournalClassical and Quantum Gravity (0264-9381), 37(4), 045006 ~ -
  • Enrollment typeSCIE
  • publication date 20200116
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 neutron stars.