Credit & Copyright: X-ray;
J. Liu (U.Mich.)
et al.,
CXC,
NASA
-
Optical;
T. Boroson
(NOAO),
AURA,
NOAO,
NSF
Explanation:
In visual appearance, M74 is a
nearly perfect face-on spiral
galaxy, about 30 million light-years away toward the
constellation Pisces.
The red blotches seen in
this
composite view are ultraluminous
x-ray sources (ULXs) mapped by the
Chandra X-ray Observatory.
The ULXs are so called because they actually do radiate 10 to
1,000 times more x-ray power than "ordinary"
x-ray binary stars,
which harbor a neutron star or
stellar mass
black hole.
In fact,
watching
these ULXs change their
x-ray brightness over periods of 2 hours or so, astronomers
conclude that ULXs could well be
intermediate mass black holes --
black holes with
masses 10,000 times or so greater than the Sun, but still much less
than the million solar mass black holes which
lurk in the centers
of large spiral galaxies.
How did these intermediate mass black holes get there?
One intriguing suggestion is that they are left over from
the cores of much smaller galaxies that are
merging with
spiral galaxy M74.
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Publikacii s klyuchevymi slovami:
M 74 - spiral galaxy - black hole - spiral'naya galaktika - rentgenovskoe izluchenie - chernye dyry
Publikacii so slovami: M 74 - spiral galaxy - black hole - spiral'naya galaktika - rentgenovskoe izluchenie - chernye dyry | |
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