Previous X-ray observations had hinted that the gas was not moving uniformly
across the cluster as might be expected.
Using the superior sensitivity and spectral resolution of the XMM-Newton and
Chandra X-ray telescopes, Dupke took readings from two locations in the cluster
and saw that there was a distinct difference in the velocity of the gas. One
part of the cluster seemed to be moving away from Earth faster than the other.
According to the researchers it was puzzling because the moving gas was cold
by astronomical standards. If this gas moved at such high speeds, it should have
had a temperature of more than double the measured 50 million degrees Celsius.
Dupke realised that Abell 576 is undergoing a collision, but seen head on, so
that one cluster is now almost directly behind the other.
The 'cold' clouds of gas are the cores of each cluster, which have survived
the initial collision but will eventually fall back together to become one.
The data reveals that the clusters have collided at a speed of over
3,300km/s. This is "interesting" because there are some computer models of
colliding galaxy clusters which suggest that such a high speed is impossible to
reach.
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