Galaxienhaufen enthalten dünnes, heißes, im Röntgenbereich strahlendes Gas zwischen ihren Galaxien.
In den meisten Haufen ist dieses Gas kugelsymmetrisch verteilt.
Doch in den Haufen mit Relikten wurden starke Deformationen der Gasverteilung beobachtet (Abbildung 1).
www.mpa-garching.mpg.deClusters of galaxies contain dilute and hot, X-ray emitting gas in the space between the galaxies.
In most clusters this gas is symmetrically distributed about their centres.
However, it was observed that clusters that host radio relics show strong deformations (see Fig.
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