Investigating close binary supermassive black holes at high angular resolution
Gravitational waves (GW) in the nano-Hz domain are expected to be radiated by close-binaries of supermassive black holes (CB-SMBHs; components bound in a Keplerian binary at mutual distance less than ~ 0.1 pc), which are relicts of galaxy mergers and anticipated to be measured via the Pulsa...
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| Формат: | Статья |
| Язык: | English |
| Опубликовано: |
Astronomical Observatory, Department of Astronomy, Belgrade
2021-01-01
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| Серии: | Serbian Astronomical Journal |
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| Online-ссылка: | http://www.doiserbia.nb.rs/img/doi/1450-698X/2021/1450-698X2102001K.pdf |