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Super-massive black hole binaries in gas-rich environments
Published online by Cambridge University Press: 17 July 2013
Abstract
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.†
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 265
- Copyright
- Copyright © International Astronomical Union 2013