thanks Smallphi,
here is the article about that, published in Astrophysical Journal
http://arxiv.org/abs/0706.3048
A Dark Core in Abell 520
A. Mahdavi (UVic), H. Hoekstra (UVic), A. Babul (UVic), D. Balam (UVic), P. Capak (Caltech)
10 pages, 5 figures
(Submitted on 21 Jun 2007)
"The rich cluster Abell 520 (z=0.201) exhibits truly extreme and puzzling multi-wavelength characteristics. It may best be described as a "cosmic train wreck." It is a major merger showing abundant evidence for ram pressure stripping, with a clear offset in the gas distribution compared to the galaxies (as in the bullet cluster 1E 0657-558). However, the most striking feature is a massive dark core (721 h_70 M_sun/L_sun) in our weak lensing mass reconstruction. The core coincides with the central X-ray emission peak, but is largely devoid of galaxies. An unusually low mass to light ratio region lies 500 kpc to the east, and coincides with a shock feature visible in radio observations of the cluster. Although a displacement between the X-ray gas and the galaxy/dark matter distributions may be expected in a merger, a mass peak without galaxies cannot be easily explained within the current collisionless dark matter paradigm. Interestingly, the integrated gas mass fraction (~0.15), mass-to-light ratio (220 h_70 M_sun/L_sun), and position on the X-ray luminosity-temperature and mass-temperature relations are unremarkable. Thus gross properties and scaling relations are not always useful indicators of the dynamical state of clusters."
My take on it is: here's another cluster collision aftermath where they have now mapped where the dark matter is, and mapped where the X-ray gas is, etc. And they are trying to reconstruct what happened during the collision.
they tried to fit MOND but said it was hopeless
I guess "trainwreck" could be considered as more evidence for the existence of dark matter, giving still more information about how it behaves. Still don't know what it is or the extent of its interaction. every weak-lensing map they make of it gives additional information
and yes, it doesn't always behave the way the simple theory of its behavior says it should, apparently----so the plot thickens