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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| Format: | Article |
| Langue: | English |
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Astronomical Observatory, Department of Astronomy, Belgrade
2021-01-01
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| Collection: | Serbian Astronomical Journal |
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| Accès en ligne: | http://www.doiserbia.nb.rs/img/doi/1450-698X/2021/1450-698X2102001K.pdf |