Where have all the quasars gone?
Published: December 5, 2011
An international team of astronomers has discovered two gigantic black holes with masses about 10 billion times the mass of our sun. These black holes have a mass more than 50 per cent greater than any other previously measured.
“They may be the dormant remains of quasars that were extremely luminous billions of years ago,” said Professor James Graham, director of the Dunlap Institute for Astronomy and Astrophysics at the University of Toronto and founding member of the team behind the discovery.
A black hole is a region of space that has so much mass concentrated in it that there is no way for a nearby object to escape its gravitational pull. The masses of black holes are measured by figuring out how strong their gravity is. More mass means more gravity and a stronger effect on stars that orbit in the galaxies that they inhabit.
Using several telescopes − the Gemini Observatory, the MacDonald Observatory and the Keck Observatory – the scientists measured the speed of stars orbiting in these galaxies, thereby measuring the strength of the gravitational field of the black hole.
“Black holes inhabit the centres of nearly all galaxies − the centre of our very own Milky Way galaxy harbours a black hole four million times the mass of the sun − relatively speaking, a baby! But only a few dozens of these black holes have been ‘weighed’ carefully,” said Graham.
“We believe that 10-billion solar mass black holes like these are the ultimate power sources for the distant quasars observed in the early universe, one to three billion years after the Big Bang,” he said.
Quasars are among the brightest phenomena in the universe, emitted by material whirling around and falling into the black hole at the centre of a galaxy. The more massive the black hole, the more powerful the quasar can be.
More recently, quasars have toned it down: the ones closer to home are not nearly as luminous as those of 10 billion years ago. The light coming from the two galaxies the team observed shows them as they were less than half a billion years ago. No quasar there, but black holes massive enough to have powered extremely bright quasars several billions of years earlier.
“Our measurements of black holes with 10-billion solar masses in nearby galaxies show that these types of galaxies originally hosted very luminous quasars,” said Graham. “For the last 10 billion years, these enormous black holes have been dormant.”
To look for such massive black holes, the team turned their telescopes toward giant galaxies since there appears to be a tight correlation between properties of the host galaxy and the mass of its black hole. This key piece of evidence helps scientists piece together how galaxies and their central black holes form and grow. The correlation suggests there is a sort of feedback between the growth of the central black hole and the formation of the stars that eventually comprise the central region of the galaxy.
“But these newly measured black hole masses are a surprise,” said Graham. “They are significantly more massive than predicted using the previously known correlations. Something that we had not anticipated for the most massive black holes must be at play here.”
Graham’s research career includes an impressive list of astronomy firsts. He discovered the first disk of asteroidal debris orbiting a white dwarf star. He made the first images of the binary black holes in the ultra-luminous galaxy Arp 220. In 1994, he was a member of a team which made one of the first definitive identifications of a brown dwarf in the Pleiades open cluster, an accomplishment that was also one of the first important discoveries made using the Keck telescope.
In 2008, he and his Berkeley colleague Paul Kalas discovered Fomalhaut b, the first exoplanet seen with visible light. Captured by the Hubble Space Telescope, the image was named one of the 10 biggest scientific breakthroughs of all time by Time magazine. Currently, Graham is working to detect many more planets by direct imaging. He is the project scientist for the Gemini Planet Imager, a highly advanced adaptive optics instrument at the Gemini Observatory in Chile.
The black hole research will be published in Nature on Dec. 8.
The illustration and Nature paper are availalbe Watch the Dunlap Institute's .
Other members of the international team include lead authors Chung-Pei Ma, Nicholas McConnell, a former student of Graham’s, and Shelley Wright, all of UC Berkeley (Wright will join οin January 2012). Research was supported by the National Science Foundation, the Hubble Fellowship, NASA, and the Miller Institute for Basic Research in Science at UC Berkeley. The Gemini Observatory is operated by the Association of Universities for Research in Astronomy, Inc. under a cooperative agreement with National Science Foundation on behalf of the Gemini partnership.
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