Youjun Lu and Chang-Shuo Yan at National Astronomical Observatories of Chinese Academy of Sciences and their collaborators found a supermassive binary black hole hiding at the center of Markarian 231, the nearest galaxy to Earth that hosts a Quasar. This work is published in the Astrophysical Journal (Yan, Lu, Dai, & Yu 2015, ApJ, 809, 117; DOI: 10.1088/0004-637X/809/2/117). 

Search for binary black holes is of great importance not only for a deep understanding of the formation and evolution of galaxies but also for further investigating the gravitational wave radiation and testing the gravity theory. Observations show that most galaxies, if not all, host supermassive black holes in their centers. In the standard galaxy formation model, a big galaxy is assembled through merger and collision of two small galaxies. The two central supermassive black holes fall into orbit about one to another as a result of the merger and generate tremendous amount of gravitational wave radiation at the end of the orbiting. In the mean time, the merger can cause the gas in the two small galaxies, if gas rich, sinking into the center of the merged galaxy and triggers a brilliant Quasar there. Astrophysicists expect the existence of binary black holes in many of those brilliant Quasars. However, the evidence is still ambiguous and uncertain.  

A research team, including Chang-Shuo Yan and Youjun Lu at National Astronomical Observatories of Chinese Academy of Sciences, Xinyu Dai at University of Oklahoma, and Qingjuan Yu at Kavli Institute for Astronomy and Astrophysics-Peking University, investigated the optical-ultraviolet continuum spectrum from the core of Markarian 231 (see Figure 1), obtained by the Hubble Space telescope and some ground based optical telescope such as Keck. They found that the “surprising and extreme feature”, a deficit, in the optical to ultraviolet continuum of Markarian 231, is best explained by a model involved a supermassive binary black hole (see Figure 2 for illustration). 

If only one black hole were present in the center of the quasar, the whole accretion disk made of surrounding hot gas would glow in ultraviolet rays. Instead, the ultraviolet glow of the gaseous disk abruptly drops off toward the center. This provides observational evidence that the disk has a big donut hole encircling the central black hole. The best explanation for the observational data, based on dynamical models, is that the center of the disk is carved out by the action of two black holes orbiting each other. (See an artist illustration picture of the system in Figure 3.) The central black hole is estimated to be 150 million times the mass of our sun, and the companion weighs in at 4 million solar masses.  The second, smaller black hole orbits in the inner edge of the accretion disk, and has its own mini-disk with an ultraviolet glow. The dynamic duo completes an orbit around each other every 1.2 years. The binary black holes are predicted to spiral together and collide within a few hundred thousand years. 

 “We are extremely excited about this finding because it not only shows the existence of a close binary black hole in Mrk 231, but also paves a new way to systematically search binary black holes via the nature of their ultraviolet light emission,” said Youjun Lu of the National Astronomical Observatories of Chinese Academy of Sciences. 

“The structure of our universe, such as those giant galaxies and clusters of galaxies, grows by merging smaller systems into larger ones, and binary black holes are natural consequences of these mergers of galaxies,” added co-investigator Xinyu Dai of the University of Oklahoma.  

The lower-mass black hole is the remnant of a smaller galaxy that merged with Markarian 231, located only about 600 million light-years away from the earth. Evidence of a recent merger comes from the host galaxy’s asymmetry, and the long tidal tails of young blue stars. The result of the merger has been to make Markarian 231 an energetic starburst galaxy with a star formation rate 100 times greater than that of our Milky Way galaxy. The infalling gas fuels the black holes’ “engine”, triggering outflows and gas turbulence that incites a firestorm of star birth. 

This finding is reported by the new center of the Hubble space telescope on August 27, 2015 and is highlighted by the AAS Nova on August 24, 2015. For more information, see http://www.nasa.gov ，http://hublesite.org/news/2015/31，and http://aasnova.org/2015/08/24/hidden-pair-of-supermassive-black-holes/

Figure 1：Image of Markarian 231 by the Hubble space telescope。 (Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA)- ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)) 

Figure 2：An illustration of the optical-to-ultraviolet continuum spectrum of Markarian 231 and the model. (Credit: NASA, ESA, and P. Jeffries (STScI)) 

 Figure 3：An artist illustration picture of the binary black hole system (Credit: NASA, ESA, and G. Bacon)