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Our group at
the Open University studies microquasars in our Galaxy. These are
objects composed of a normal star orbiting around a black hole (see
Figure 1). They are amongst the strangest, most fascinating objects
in the Universe. A black hole is a very compact object, whose gravity
is highly attractive and into which some matter falls, but from
which nothing can escape, not even light.
In these binary
systems, the black hole can attract (by gravity) matter from the
star nearby. Since matter in orbit cannot directly fall onto this
compact object, it will spiral for a long time, until it crosses
the event horizon of the black hole, after which it is lost for
ever and cannot be observed anymore. Before it crosses the event
horizon, matter accumulates in an accretion disc. From time to time,
part of the matter of the star that is attracted by the black hole
is swallowed and the rest is ejected by an unknown mechanism.
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Figure 1
Schematic
diagrams of microquasars (left) and quasars (right)
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