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3C442A: Galaxy Collision Causes Role Reversal
Astronomers think that there are enormous black holes at the centers of most, if not all, galaxies. These black holes, which can be millions or even billions of times more massive than the Sun, can greatly affect the galaxy and the environments around them. One way such black holes shape
their surroundings is by generating powerful jets of high-energy particles.
The jets, which are bright in radio waves, have been seen to push around
the hot gas that envelops the galaxy. When this happens, astronomers can
detect huge cavities and powerful shock fronts in the hot, X-ray emitting
gas.
However, the opposite scenario is apparently unfolding in the galaxy known
as 3C442A. X-ray data from NASA's Chandra X-ray Observatory and radio
observations from the NSF's Very Large Array show that the hot gas (blue)
in the middle of 3C442A is pushing apart the radio-bright gas (orange). The
inner sections of the radio structure are sharp and concave, which is
consistent with the idea that the X-ray bright gas is sweeping the
radio-emitting gas aside. This is the first convincing evidence for such a
role reversal.
A team of scientists, led by Diana Worrall of University of Bristol, UK,
has studied this system and determined why the dynamics in 3C442A seem to
be topsy-turvy. First, there are two galaxies near the middle of 3C442A
which are in the process of merging. These two galaxies are on their
second pass toward a collision, having already experienced a close
encounter. The energy generated from this impending merger is heating the
combined atmospheres from these two galaxies, causing them to shine
brightly in X-rays and expand.
The researchers determined that the jets that had produced the lobes of
radio-emitting gas are no longer active. The jets may have ceased at the
time of, and possibly as a result of, the galaxy collision. Since the
radio-emitting gas no longer has a power source, it is then at the mercy
of the expanding hot gas and has been pushed aside.
| Fast Facts for 3C442A: |
| Credit |
X-ray: NASA/CXC/Univ. of Bristol/Worrall et al.; Radio: NRAO/AUI/NSF |
| Scale |
Image is 22 by 13 arcmin |
| Category |
Quasars & Active Galaxies |
| Coordinates (J2000) |
RA 22h 14m 47.00s | Dec +13 46' 16.00" |
| Constellation |
Pegasus |
| Observation Dates |
4 pointings between July 2005 - January, 2006
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| Observation Time |
28 hours |
| Obs. IDs |
5635, 6353, 6359, 6392
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| Color Code |
X-ray (blue); Radio (orange) |
| Instrument |
ACIS |
| References | The Effect of a Chandra-measured Merger-related Gas Component on the Lobes of a Dead Radio Galaxy. Worral, D.M., Birkinshaw, M., Kraft, R.P., Hardcastle, M.J., 2007, ApJ, 685, 79 |
| Distance Estimate |
About 390 million light years |
| Release Date |
March 29, 2007 |
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