Little middle ground for black holes
Data from far off star cluster suggests cosmos holds few, if any, mid-sized black holes.
Web edition : Wednesday, August 20th, 2008
font_down font_up Text Size
access
EVERYDAY CLUSTERPictured is the globular cluster M92 in the Hercules constellation. It was thought that such clusters would host mid-sized black holes, yet to be observed. But a recent look at another globular cluster revealed that its black hole was a tiny one. Black holes perhaps come only in small or large sizes. Read more.Achut Reddy, Flynn Haase, NOAO, AURA, NSF

Fingerprinting the light emanating from a cluster of stars in the constellation Virgo reveals that the glob harbors only a tiny black hole, astronomers report in the Aug. 20 Astrophysical Journal Letters.

As cosmic garbage cans, black holes are regions of space so massive that their gravity prevents even light from escaping their pull. For several years, theorists have posited that the most likely place to find a medium-sized black hole — one weighing thousands of times more than the sun — would be at the center of a globular cluster. These clusters are gaggles of hundreds of thousands of stars and act as down-sized versions of galaxies.

The heftiest black holes are up to billions of times the mass of the sun and lie at the heart of almost all galaxies. The least massive black holes, which are about 10 times the mass of the sun, form when massive stars blow up in supernova explosions. Mid-sized black holes are thought to form when small black holes sink to the center of a globular cluster and acquire mass.

But, to date, no one has been able to find those mid-scale black holes.

To find the mass of one particular cluster’s black hole, Stephen Zepf of Michigan State University in East Lansing and an international team of astronomers studied the light emanating from the globular cluster RZ2109. This particular cluster, the team reports, contains a tiny black hole only 10 times the mass of the sun.

“That cluster is a fairly normal globular cluster,” says Zepf, lead author of the study. “So if intermediate black holes are common in globular clusters, then we have no understanding as to why there would not be in this one.”

Because RZ2109 hosts only a tiny black hole, the team concluded that similar small-sized black holes would be found in other clusters and that intermediate black holes are probably rare in globular clusters. If middle-sized black holes do exist, the cosmic garbage cans are probably lurking in satellite galaxies such as the ones that orbit the Milky Way. But right now, Zepf says, “it is just too hard to tell.”


Found in: Atom & Cosmos
Comments 2
  • Make that a 40,000 solar-mas BH in Omega Cen & the paper referenced to NGC 2808 is arXiv:0808.2661.
    Jon Hanford Jon Hanford
    Aug. 26, 2008 at 1:41pm
  • Recent observations of Omega Centauri (NGC 5139) claim to have found a 40,0000 solar-mas BH at its' center (arXiv:0801.2782)while a similar recent study of NGC 2808 finds no BH at its' center up to a limit of 140 solar masses. Other recent searches for IMBHs in 47 Tucanae, M 32, G1 in Andromeda and other nearby globular clusters have produced equivocal results. I think the jury is still out on this issue of the existence of IMBHs.
    Jon Hanford Jon Hanford
    Aug. 26, 2008 at 1:38pm
Post a comment

Please login or register to participate.


Advertisement
Suggested Reading:
seperator
Citations & References:
seperator
  • Zepf, S.E. et. al. Very Broad [O iii] λλ4959, 5007 Emission from the NGC 4472 Globular Cluster RZ 2109 and Implications for the Mass of Its Black Hole X-Ray Source. The Astrophysical Journal Letters, 683:L139–L142, 2008 August 20. arXiv:0805.2952v2
Reader Favorites:
seperator
SN on the Web:
seperator