• AuthorB.P. Abbott et al.,김환선,손재주,오상훈,오정근
• JournalThe Astrophysical Journal (0004-637X), 875, 160:1 ~ 160:19
• Enrollment typeSCI
• publication date 20190425

One unanswered question about the binary neutron star coalescence GW170817 is the nature of its post-merger remnant. A previous search for post-merger gravitational waves targeted high-frequency signals from a possible neutron star remnant with a maximum signal duration of 500 s.