Binary Supermassive Black Holes Common –Light Up Galaxies Like a Christmas Tree


To date, astronomers have discovered 33 binary black holes in distant galaxies located at distances 4 to 7 billion light-years away from Earth. This result is particularly important because it shows that supermassive black hole pairs are more common than previously known from observations, and because the black hole pairs can be used to estimate how often galaxies merge with each other.

A team of astronomers discovered that the two bright nuclei near the center of the galaxy shown avove correspond to two supermassive black holes shining as Active Galactic Nuclei.

Astronomical observations have shown that nearly every galaxy has a central supermassive black hole (with a mass of a million to a billion times the mass of the Sun), and that galaxies commonly collide and merge to form new, more massive galaxies. As a consequence of these two observations, a merger between two galaxies should bring two supermassive black holes to the new, more massive galaxy formed from the merger.

The two black holes gradually inspiral toward the center of this galaxy, engaging in a gravitational tug-of-war with the surrounding stars. The result is a black hole waltz, which is expected to occur in our own Milky Way Galaxy in about 3 billion years, when it collides with the Andromeda Galaxy.

Astronomers expect there to be many such waltzing supermassive black holes in the Universe, but until recently only a handful had been found. Dr. Comerford and her colleagues announce the discoveries of 33 new pairs of waltzing supermassive black holes, which help alleviate the discrepancy between the expected and observed numbers of black hole pairs.

Dr. Comerford and her colleagues observed the waltzing black holes that have gas collapsing onto them, and this gas releases energy and powers each black hole as an active galactic nucleus (AGN). This lights up the black hole like a Christmas tree.

By searching for the redshifted and blueshifted light that is a signature of black hole dances, Dr. Comerford and her colleagues discovered 32 waltzing supermassive black hole pairs in the DEEP2 Galaxy Redshift Survey, a survey of 50,000 galaxies observed with the Deep Imaging Multi-Object Spectrograph (DEIMOS) on the 10-meter (400-inch) Keck II Telescope on Mauna Kea, Hawaii.

The team clocked each black hole dance at a velocity of a few hundred kilometers per second (500,000 miles per hour) and in each case measured the distance between the two black hole dancers to be 3000 lightyears (1/8 the distance from the Sun to the center of the Milky Way Galaxy).

The team developed their second technique for identifying the black holes through a chance discovery of a curious looking galaxy. While visually inspecting images of galaxies taken with the Advanced Camera for Surveys on the Hubble Space Telescope, the team noticed a galaxy with a tidal tail of stars, gas, and dust, an unmistakable sign that the galaxy had recently merged with another galaxy, and the galaxy also featured two bright nuclei near its center.

The team recognized that the two bright nuclei might be the AGNs of two waltzing black holes, a hypothesis seemingly supported by the recent galaxy merger activity evinced by the tidal tail.

To test this hypothesis, the very next night the team obtained a spectrum of the galaxy with the DEIMOS spectrograph on the 10-meter (400-inch) Keck II Telescope on Mauna Kea, Hawaii.
The spectrum showed that the two central nuclei in the galaxy were indeed both AGNs, supporting the team’s hypothesis that the galaxy has two supermassive black holes. The black holes may be waltzing within the host galaxy, or the galaxy may have a recoiling black hole kicked out of the galaxy by gravity wave emission; additional observations are necessary to distinguish between these explanations.

The galaxy, called COSMOS J100043.15+020637.2, is part of the Cosmological Evolution Survey (COSMOS) and is located at a distance 4 billion light-years away from Earth (corresponding to a look-back time of 4 billion years; when the Universe was 10 billion years old). The team measured that the distance between the two black holes is 8000 light-years (1/3 the distance from the Sun to the center of the Milky Way Galaxy).

Using the techniques of searching for waltzing supermassive black holes by their velocities and obtaining spectra of galaxies that show two bright central nuclei and evidence of recent galaxy mergers, Dr. Comerford and her colleagues discovered a total of 33 pairs of supermassive black holes in distant galaxies.

These discoveries are significant because “they show that dual supermassive black hole systems are much more common than previously known from observations,” says Dr. Comerford, who is a postdoctoral researcher in astrophysics at the University of California, Berkeley. The dual supermassive black hole pairs can in turn be used to estimate how often galaxies merge, and the team concludes that red galaxies from between 4 and 7 billions years ago underwent 3 mergers every billion years.

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Image Credit: Credit: NASA/ESA


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