RAS PN 08/46: An upper mass limit for black holes?
ROYAL ASTRONOMICAL SOCIETY PRESS INFORMATION NOTE
Date: 7th September 2008
For Immediate Release
Ref.: PN 08/46
Suzanne Taylor Muzzin
Yale University Science News
Office of Public Affairs
Tel: +1 203/432-1345
Fax: +1 203/432-1323
RAS PN 08/46: AN UPPER MASS LIMIT FOR BLACK HOLES?
There appears to be an upper limit to how big the Universe's most massive black holes can get, according to new research led by a Yale University astrophysicist and published in Monthly Notices of the Royal Astronomical Society.
Once considered rare and exotic objects, black holes are now known to exist throughout the Universe, with the largest and most massive found at the centres of the largest galaxies. These "ultra-massive" black holes have been shown to have masses upwards of one billion times that of our own Sun. Now, Priyamvada Natarajan, an associate professor of astronomy and physics at Yale University and a fellow at the Radcliffe Institute for Advanced Study, has shown that even the biggest of these gravitational monsters can't keep growing forever. Instead, they appear to curb their own growth - once they accumulate about 10 billion times the mass of the Sun.
These ultra-massive black holes, found at the centres of giant elliptical galaxies in huge galaxy clusters, are the biggest in the known Universe. Even the large black hole at the centre of our own Milky Way galaxy is thousands of times less massive than these behemoths. But these gigantic black holes, which accumulate mass by sucking in matter from neighbouring gas, dust and stars, seem unable to grow beyond this limit regardless of where - and when - they appear in the Universe. "It's not just happening today," said Natarajan. "They shut off at every epoch in the Universe."
The study, which appears in the Monthly Notices of the Royal Astronomical Society (MNRAS) on 15 October, represents the first time an upper mass limit has been derived for black holes. Natarajan used existing optical and X-ray data of these ultra-massive black holes to show that, in order for those various observations to be consistent, the black holes must essentially shut off at some point in their evolution.
One possible explanation put forth by Natarajan is that the black holes eventually reach the point when they radiate so much energy as they consume their surroundings that they end up interfering with the very gas supply that feeds them, which may interrupt nearby star formation. The new findings have implications for the future study of galaxy formation, since many of the largest galaxies in the Universe appear to co-evolve along with the black holes at their centres.
"Evidence has been mounting for the key role that black holes play in the process of galaxy formation," said Natarajan. "But it now appears that they are likely the prima donnas of this space opera."
The authors of the paper are Priyamvada Natarajan (Yale University and the Radcliffe Institute for Advanced Study) and Ezequiel Treister (European Southern Observatory, Chile and University of Hawaii).
CONTACTS AND FURTHER INFORMATION
Suzanne Taylor Muzzini
Yale University Science News (details above)
Dr Robert Massey
Press and Policy Officer
Royal Astronomical Society
London W1J 0BQ
Tel: +44 (0)794 124 8035, +44 (0)20 7734 4582
Priyamvada Natarajan home page
NOTES FOR EDITORS
The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.