Rymer
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matt.o said:But hang on, it is known that the majority of the normal (baryonic) matter within a cluster does not reside in the galaxies or, by extension, black holes (see Chalnoth's post regarding the mass of a galaxy's black hole compared with its overall mass). The majority of the mass is in the gas (the hot, X-ray emitting gas Chandra sees). In fact, the gas mass dominates the galaxy stellar mass by about a factor of 5. However, for the Bullet cluster, the lensing maps clearly show that the mass centroids correspond to where the galaxies are (i.e. where the majority of the baryonic mass is not) and that this is clearly offset from the gas, which is collisional, and has become separated from the collisionless galaxies during the merger. This strongly implies that there is a dominant collisionless mass component carrying the galaxies along with it.
Which super-massive objects? The clusters themselves have masses ~10^{15} times the mass of the sun.
I'm not really disagreeing with any of that -- they also state that these 'outside' areas of mass are on the expected course lines of the clusters as if there were no 'collision'. My point is simply, there are a lot of supermassive components in a cluster, many will be near the center and some scattered throughout the cluster. So my expectation would be that these objects would just continue on -- mostly uneffected. Likely there would be a concentration of such from the central zone -- but also from throughout the cluster.
So how can the properties of this material be determined -- and that its not baryonic?