This composite image
of a galaxy illustrates how the intense gravity of a supermassive
black hole can be tapped to generate immense power. The image
contains X-ray data from NASA's Chandra X-ray Observatory (blue),
optical light obtained with the Hubble Space Telescope (gold) and
radio waves from the NSF's Very Large Array (pink).
This multi-wavelength view shows 4C+29.30, a galaxy
located some 850 million light years from Earth. The radio emission
comes from two jets of particles that are speeding at millions of
miles per hour away from a supermassive black hole at the center of
the galaxy. The estimated mass of the black hole is about 100
million times the mass of our Sun. The ends of the jets show larger
areas of radio emission located outside the galaxy.
The X-ray data show a different aspect of this galaxy,
tracing the location of hot gas. The bright X-rays in the center of
the image mark a pool of million-degree gas around the black hole.
Some of this material may eventually be consumed by the black hole,
and the magnetized, whirlpool of gas near the black hole could in
turn, trigger more output to the radio jet.
Most
of the low-energy X-rays from the vicinity of the black hole are
absorbed by dust and gas, probably in the shape of a giant doughnut
around the black hole. This doughnut, or torus blocks all the
optical light produced near the black hole, so astronomers refer to
this type of source as a hidden or buried black hole. The optical
light seen in the image is from the stars in the galaxy.
The bright spots in X-ray and radio emission on the outer
edges of the galaxy, near the ends of the jets, are caused by
extremely high energy electrons following curved paths around
magnetic field lines. They show where a jet generated by the black
hole has plowed into clumps of material in the galaxy (mouse over
the image for the location of these bright spots). Much of the
energy of the jet goes into heating the gas in these clumps, and
some of it goes into dragging cool gas along the direction of the
jet. Both the heating and the dragging can limit the fuel supply
for the supermassive black hole, leading to temporary starvation
and stopping its growth. This feedback process is thought to cause
the observed correlation between the mass of the supermassive black
hole and the combined mass of the stars in the central region or
bulge of a galaxy.
More at http://chandra.harvard.edu/photo/2013/4c2930/
-Megan Watzke, CXC
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