Chandra Finds Well-Established Black Holes In Distant Quasars (Forwarded)
Andrew Yee
Marshall Space Flight Center, Huntsville, AL March 28, 2002
Phone: 256-544-6535
Megan Watzke
Chandra X-ray Observatory Center, CFA, Cambridge, MA
Phone: 617-496-7998
cxcp...@cfa.harvard.edu
Science Contacts:
Niel Brandt, ni...@astro.psu.edu, (814) 865-3509
Smita Mathur, sm...@astronomy.ohio-state.edu, (614) 292 5779
Jill Becthold, sm...@astronomy.ohio-state.edu, (520) 621-6533
Dan Schwartz, dsch...@cfa.harvard.edu, (617) 495-7232
PIO Contacts:
Barbara Kennedy, Penn State
sci...@psu.edu, (814) 863-4682
Lori Stiles, University of Arizona
lst...@u.arizona.edu, (520) 621-1877
RELEASE: 02-04
Chandra Finds Well-Established Black Holes In Distant Quasars
Pushing further back toward the first generation of objects to form in
the Universe, NASA's Chandra X-ray Observatory has observed the three
most distant known quasars and found them to be prodigious producers
of X-rays. This indicates that the supermassive black holes powering
them were already in place when the Universe was only about one billion
years old.
"Chandra's superb sensitivity has allowed the detection of X-rays from
the dawn of the modern Universe, when the first massive black holes
and galaxies were forming," said Niel Brandt of Penn State University,
leader of one the teams involved. "These results indicate that future
X-ray surveys should be able to detect the first black holes to form
in the Universe."
The three quasars were recently discovered at optical wavelengths by
the Sloan Digital Sky Survey and are 13 billion light years from Earth,
making them the most distant known quasars. The X-rays Chandra detected
were emitted when the Universe was only a billion years old, about 7
percent of the present age of the Universe.
Since X-rays reveal conditions in the immediate vicinity of supermassive
black holes, Brandt proposed that Chandra look at these objects in three
snapshots of about two hours each to see if they were different from
their older counterparts. The observations on January 29, 2002 were made
public immediately and the four different teams quickly went to work on
them.
Brandt's team concluded that the quasars looked similar to ones that
were at least twice as old, so the conditions around the central black
hole had not changed much in that time, contrary to some theoretical
expectations. A team led by Smita Mathur of Ohio State University
reached a similar conclusion.
"These young quasars do not appear to be any different from their older
cousins, based upon our current understanding and assumptions," said
Mathur. "Perhaps the most remarkable thing about them may be that they
are so absolutely unremarkable."
Jill Bechtold of the University of Arizona and her colleagues disagree.
In addition to the three distant Sloan quasars, they observed 14 other
quasars with distances between 12 and 12.5 billion light years.
Bechtold's group looked at their larger sample to determine that the
younger, more distant quasars were radiating a lower percentage of
their energy in X-rays.
"The X-ray data are consistent with predictions of some theories that
a hot gas atmosphere is associated with the accretion disk swirling
around a central supermassive black hole," said Bechtold, provided
the distant quasars have more massive black holes than nearby ones.
"These theories predict that large supermassive black holes should be
relatively weaker X-ray emittters than smaller ones, which is what we
observed with Chandra.
All groups agreed that the masses of the black holes producing the
X-rays are huge, given their relative youth. By various estimates,
the three quasars each weighed in at between one and 10 billion times
the mass of the Sun. By comparison, the black hole at the center of
the Milky Way is believed to contain the mass equivalent to only
about 3 million Suns.
Daniel Schwartz of the Harvard-Smithsonian Center for Astrophysics
took a different approach to the same data. In addition to looking
at the quasars themselves, he examined the space around them. His
search paid off with the discovery of a new X-ray source, which may
be only about half a million light years away from the quasar
SDSS 1306+0356
"It's not clear what the source is," said Schwartz. "One plausible
explanation is that it is due to a high energy jet of material
ejected by the quasar over at least several hundred thousand years."
Chandra has detected a number of such jets, which could be generated
by the extraction of energy from the rotation of a supermassive
black hole.
In addition to SDSS 1306+0356, which has a cosmological redshift
z = 5.99, the other distant Sloan Digital Sky Survey quasars
observed in this study are SDSS 0836+0054 (redshift z = 5.82) and
SDSS 1030+0524 (redshift z = 6.28). The paper from Brandt et al has
been published in The Astrophysical Journal Letters, and Mathur et
al and Schwartz et al will have in separate papers appearing shortly
in same publication; the work of Bechtold et al will be published in
The Astrophysical Journal.
These observations were made with Chandra's Advanced CCD Imaging
Spectrometer, which was conceived and developed for NASA by Penn State
and the Massachusetts Institute of Technology. NASA's Marshall Space
Flight Center in Huntsville, Ala., manages the Chandra program, and
TRW, Inc., Redondo Beach, Calif., is the prime contractor for the
spacecraft. The Smithsonian's Chandra X-ray Center controls science
and flight operations from Cambridge, Mass.
[NOTE: Images supporting this release are available at
http://chandra.harvard.edu/photo/2002/highzqso/index.html
or
http://www1.msfc.nasa.gov/NEWSROOM/news/photos/2002/photos02-068.htm]
--
Andrew Yee
ay...@nova.astro.utoronto.ca