
Image courtesy NASA and John Mulchaey
|
Until now astronomers thought that old, red cluster galaxies were
past their prime and subdued. Only about 1 percent were supposed to
have Active Galactic Nuclei (AGN)violent centers where supermassive
black holes gobble up surrounding material and emit it as X-rays.
A surprising find by a team of Carnegie astronomers, led by Starr
Fellow Paul Martini at the Observatories, has changed this view. Using
a combination of space-based X-ray and Earth-based optical instrumentation,
the scientists found that six times the expected number of galaxies
in a nearby cluster have active centers. This alters our view
of galaxy clusters as the retirement homes for old and quiet black
holes, said team member Dan Kelson. The question now is,
How do these black holes turn themselves on again? The discovery
has also brought into question how galaxies evolve and how stars form
in these environments.
The Carnegie group, which also included John Mulchaey and Scott
Trager, published their results in the September 10 issue of
Astrophysical Journal Letters. They took an unusual approach
to their study by using NASAs X-ray Chandra satellite
in concert with Carnegies new 6.5-meter Walter Baade optical
telescope at the Las Campanas Observatory in Chile. Using the Chandra
data, they discovered six X-ray sources in galaxy cluster Abell
2104, about 700 million light-years from Earth.
|
They then used the Carnegie telescope to confirm that all of the
galaxies are in the cluster and not in the foreground or background.If
we had used optical data alone, we would have missed these hidden
monsters, said John Mulchaey.If wed used only
X-ray data, we would not have been sure that all the AGNs were in
the cluster.
Galaxy clusters typically have hundreds to thousands of galaxy
members. The researchers surveyed the 100 brightest galaxies in
Abell 2104. It is believed that old, red galaxies generally populate
clusters because during cluster formation the raw material for making
stars and feeding black holesgasis burned off and nothing
is left to fuel these systems. The presence of these AGNs
indicates that supermassive black holes have somehow retained a
fuel source, said Martini. Despite the harsh treatment
these galaxies suffered as a cluster, they seem to be having the
black hole equivalent of a midlife crisis. They aren't over the
hill after all. The group has already started studying other
clusters to see if similar activity is present elsewhere.
This is a false-color
X-ray of the Abell 2104 cluster of galaxies taken with NASAs
Chandra X-ray Observatory overlaid on an optical image taken with
Carnegies 6.5-meter Walter Baade telescope in Las Campanas,
Chile. The image reveals X-ray emissions produced both by hot gas
(the blue area near the center of the image)
and by accretion of dust and gas onto supermassive black holes (the
smaller blue patches on the outer edges of the image). The number
of active, supermassive black holes found in this cluster is six
times the amount found using other techniques. The finding suggests
that active black holes are much more common in clusters of galaxies
than previously believed.
|