Abstract
We still do not know the timescale for the merging of binary black holes (BHs). This timescale has important implications for gravitational wave predictions and our understanding of BH demographics. Here we discuss efforts to constrain the fraction of BH pairs on kpc scales using observations of dual active galactic nuclei.
Original language | English (US) |
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Pages (from-to) | 299-305 |
Number of pages | 7 |
Journal | Proceedings of the International Astronomical Union |
Volume | 11 |
Issue number | A29B |
DOIs | |
State | Published - 2015 |
All Science Journal Classification (ASJC) codes
- Medicine (miscellaneous)
- Astronomy and Astrophysics
- Nutrition and Dietetics
- Public Health, Environmental and Occupational Health
- Space and Planetary Science
Keywords
- active galactic nuclei
- binary black holes
- supermassive black holes