• 저자B. P. Abbott,김환선,손재주,오상훈,오정근
• 학술지The Astrophysical Journal (0004-637X), 883(2), 149-1 ~ 149-10
• 등재유형SCI
• 게재일자 20190930

When formed through dynamical interactions, stellar-mass binary black holes (BBHs) may retain eccentric orbits (e > 0.1 at 10 Hz) detectable by ground-based gravitational-wave detectors.