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Super-massive black hole binaries in gas-rich environments
2012
Proceedings of the International Astronomical Union
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Black hole binaries form after major galaxy mergers, but their fate is unclear as hardening due to stars gets inefficient at sub-parsec distances. We model an alternative scenario in which the merger is driven by the interaction of the binary with the surrounding gas.†
doi:10.1017/s1743921313004985
fatcat:pjs6gggwd5dznnwjdpv5z2pq3q