Super-massive black hole binaries in gas-rich environments release_pjs6gggwd5dznnwjdpv5z2pq3q

by Jorge Cuadra

Published in Proceedings of the International Astronomical Union by Cambridge University Press (CUP).

2012   Issue S295, p265

Abstract

<jats:title>Abstract</jats:title> 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.†
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