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Massive black holes "switch on" due to galaxy collisions

Results contribute to scientists' understanding of one of the most exotic phenomena in the universe.
Provided by the Max Planck Institute, Garching, Germany
NGC 2207
Galaxy mergers — shown here is the system NGC 2207 in the constellation Canis Major — are the most likely reason why active galactic nuclei occur.
ESO
June 15, 2010
The center of most galaxies harbors a massive black hole. So does our Milky Way. The exotic object there, however, is calm, unlike some supermassive gravity monsters in other galaxies. Scientists at the Max Planck Institute for Extraterrestrial Physics in Garching, Germany, and other institutions around the world have analyzed 199 of these galaxies and discovered what makes black holes at galaxy centers become active — black holes switched on some 700 million years ago after major galaxy merger events.

While in our own galaxy the central black hole was measured to have about 4 million solar masses, the 199 galaxies analyzed host black holes with a typical mass of about 300 million solar masses. These galaxies are larger than our Milky Way and also active, which means that the inner region of the galaxy has a higher luminosity than normal.

Astronomers believe this radiation is powered by the accretion of matter on the supermassive black hole. Previous studies suggest that the formation and evolution of the host galaxies and their black holes are closely connected. However, there are various possibilities how the interstellar gas can be funneled toward the black hole, and it is unclear which of these mechanisms is dominant at what stage in the evolution of a galaxy.

The two main mechanisms discussed are either internal disruptions, such as galaxy disk instabilities, or mergers and tidal interactions between close pairs of galaxies. Simulations of these scenarios lead to different predictions about the clustering of active galaxies and the masses of the host galaxies. Previous studies have analyzed active galaxies selected by their optical or soft X-ray emission, which misses a major part of the radiation powered by the black hole accretion due to absorption and other effects.

"For our sample, we used galaxies selected by their hard X-ray emission in the Swift-BAT all-sky survey, which provides an unprecedented depth and characterizations of source properties," said Nico Cappelluti from the Max Planck Institute for Extraterrestrial Physics.

"With this survey, we have a complete sample of local active galaxies, and so we can perform the measurement of black holes and the dark matter halos which host them in our cosmological backyard," said Marco Ajello, from the Kavli Institute of Particle Astrophysics and Cosmology at Stanford University in Palo Alto, California.

The clustering analysis of the 199 galaxies gives an unbiased picture of the co-existence and evolution of galaxies and their active nuclei in the local universe. The scientists estimate that the black holes powering the active galaxies have a typical mass of about 300 million solar masses and are hosted by massive galaxies with about 200 billion solar masses residing in big bubbles of dark matter as massive as 100 Milky Ways. These properties scale with luminosity — the more luminous sources are hosted in more massive galaxies with bigger black holes.

By merging the observational evidence and theoretical model predictions, the scientists found that the most plausible scenario for the history of local active galaxies is a merger event. "The active galactic nuclei 'switch on' after a major merger event about 700 million years ago and shine brightly for the first part of their lives where they gain most of their mass," said Cappelluti. "After about 200 to 500 million years, they accrete with lower and lower efficiency as the gas reservoirs become depleted. Today, they have grown to supermassive black holes with 100 to 1,000 million solar masses and shine with moderately low luminosity compared to other active galaxies." The black holes starve as their gas supply becomes less and less.

These results give an important contribution to our understanding of the origin of supermassive black holes shining in the centers of galaxies that have been puzzling astronomers for almost a century. In the coming years, the new generation of X-ray telescopes, such as the extended ROntgen Survey with an Imaging Telescope Array (eROSITA), which is currently under construction at the Max Planck Institute for Extraterrestrial Physics, will perform further mappings of black holes and dark matter. These new studies will open up new perspectives on the history of the most exotic phenomena in the universe.
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