The X-ray light curve of the debris from a star torn apart by a supermassive black hole provides the best evidence yet for two such black holes orbiting close to each other.
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References
Kormendy, J. & Ho, L. C. Ann. Rev. Astron. Astrophys. 51, 511–653 (2013).
Begelman, M. C., Blandford, R. D. & Rees, M. J. Nature 287, 307–309 (1980).
Liu, F. K., Li, Shuo & Komossa, S. Astrophys. J. 786, 103 (2014).
Gaskell, C. M. Liége Int. Astrophys. Colloq. 24, 473–477 (1983).
Popovic, L. C. New Astron. Rev. 56, 74–91 (2012).
Gaskell, C. M. Nature 463, E1 (2010).
Hills, J. G. Nature 254, 295–298 (1975).
Rees, M. J. Nature 333, 523–527 (1988).
Phinney, E. S. IAU Symp. 136, 543–553 (1989).
Ivanov, P. B., Polnarev, A. G. & Saha, P. Mon. Not. R. Astron. Soc. 358, 1361–1378 (2005).
Liu, F. K., Li, S. & Chen, X. Astrophys. J. 706, L133–L137 (2009).
Saxton, R. D. et al. Astron. Astrophys. 541, A106 (2012).
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Gaskell, M. Together at last. Nature Phys 10, 481–482 (2014). https://doi.org/10.1038/nphys3015
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DOI: https://doi.org/10.1038/nphys3015
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