A close-pair binary in a distant triple supermassive black hole system

R P Deane¹, Z Paragi², M J Jarvis³, M Coriat¹, G Bernardi⁴, R P Fender⁵, S Frey⁶, I Heywood⁷, H-R Klöckner⁸, K Grainge⁹, C Rumsey¹⁰

Affiliations

¹ 1] Astrophysics, Cosmology and Gravity Centre, Department of Astronomy, University of Cape Town, Rondebosch, 7701, Cape Town, South Africa [2] Square Kilometre Array South Africa, Pinelands, 7405, Cape Town, South Africa.
² Joint Institute for VLBI in Europe, 7990 AA, Dwingeloo, The Netherlands.
³ 1] Astrophysics, Department of Physics, University of Oxford, Oxford OX1 3RH, UK [2] Physics Department, University of the Western Cape, Belville, 7535, South Africa.
⁴ 1] Square Kilometre Array South Africa, Pinelands, 7405, Cape Town, South Africa [2] Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown, 6140, South Africa [3] Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
⁵ Astrophysics, Department of Physics, University of Oxford, Oxford OX1 3RH, UK.
⁶ Satellite Geodetic Observatory, Institute of Geodesy, Cartography and Remote Sensing, H-1592, Budapest, Hungary.
⁷ 1] Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown, 6140, South Africa [2] Australia Telescope National Facility, CSIRO Astronomy and Space Science, Epping, New South Wales 1710, Australia.
⁸ Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany.
⁹ Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester, UK.
¹⁰ Astrophysics Group, Cavendish Laboratory, University of Cambridge, Cambridge, UK.

PMID: 24990745
DOI: 10.1038/nature13454

A close-pair binary in a distant triple supermassive black hole system

R P Deane et al. Nature. 2014.

. 2014 Jul 3;511(7507):57-60.

doi: 10.1038/nature13454. Epub 2014 Jun 25.

Authors

R P Deane¹, Z Paragi², M J Jarvis³, M Coriat¹, G Bernardi⁴, R P Fender⁵, S Frey⁶, I Heywood⁷, H-R Klöckner⁸, K Grainge⁹, C Rumsey¹⁰

Affiliations

¹ 1] Astrophysics, Cosmology and Gravity Centre, Department of Astronomy, University of Cape Town, Rondebosch, 7701, Cape Town, South Africa [2] Square Kilometre Array South Africa, Pinelands, 7405, Cape Town, South Africa.
² Joint Institute for VLBI in Europe, 7990 AA, Dwingeloo, The Netherlands.
³ 1] Astrophysics, Department of Physics, University of Oxford, Oxford OX1 3RH, UK [2] Physics Department, University of the Western Cape, Belville, 7535, South Africa.
⁴ 1] Square Kilometre Array South Africa, Pinelands, 7405, Cape Town, South Africa [2] Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown, 6140, South Africa [3] Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA.
⁵ Astrophysics, Department of Physics, University of Oxford, Oxford OX1 3RH, UK.
⁶ Satellite Geodetic Observatory, Institute of Geodesy, Cartography and Remote Sensing, H-1592, Budapest, Hungary.
⁷ 1] Centre for Radio Astronomy Techniques and Technologies, Department of Physics and Electronics, Rhodes University, Grahamstown, 6140, South Africa [2] Australia Telescope National Facility, CSIRO Astronomy and Space Science, Epping, New South Wales 1710, Australia.
⁸ Max-Planck-Institut für Radioastronomie, D-53121 Bonn, Germany.
⁹ Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester, UK.
¹⁰ Astrophysics Group, Cavendish Laboratory, University of Cambridge, Cambridge, UK.

PMID: 24990745
DOI: 10.1038/nature13454

Abstract

Galaxies are believed to evolve through merging, which should lead to some hosting multiple supermassive black holes. There are four known triple black hole systems, with the closest black hole pair being 2.4 kiloparsecs apart (the third component in this system is at 3 kiloparsecs), which is far from the gravitational sphere of influence (about 100 parsecs for a black hole with mass one billion times that of the Sun). Previous searches for compact black hole systems concluded that they were rare, with the tightest binary system having a separation of 7 parsecs (ref. 10). Here we report observations of a triple black hole system at redshift z = 0.39, with the closest pair separated by about 140 parsecs and significantly more distant from Earth than any other known binary of comparable orbital separation. The effect of the tight pair is to introduce a rotationally symmetric helical modulation on the structure of the large-scale radio jets, which provides a useful way to search for other tight pairs without needing extremely high resolution observations. As we found this tight pair after searching only six galaxies, we conclude that tight pairs are more common than hitherto believed, which is an important observational constraint for low-frequency gravitational wave experiments.

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Comment in

Astrophysics: A tight duo in a trio of black holes.
Taylor G. Taylor G. Nature. 2014 Jul 3;511(7507):35-7. doi: 10.1038/nature13511. Epub 2014 Jun 25. Nature. 2014. PMID: 24990736 No abstract available.

References

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1. Nature. 2008 Apr 17;452(7189):851-3 - PubMed

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A close-pair binary in a distant triple supermassive black hole system

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A close-pair binary in a distant triple supermassive black hole system

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