To my mind, the Bullet Cluster is actually strong evidence
against non-baryonic dark matter, and here's why:
The tightness of the Tully-Fisher Relation. Originally the TFR was observed to be a tight relation between the optical luminosity of spiral galaxies and the HI line width, which was a measure of the outer circular velocity. The scatter in the plot is about 18%, which could fairly be attributed entirely to measurement errors. So, at least within a certain mass range, the stellar population somehow
knows exactly how much dark matter there is in the galaxy (that is, if there is any there at all).
The TFR breaks down with low luminosity galaxies. However take a look at the paper I link to below. DO not be put off by the fact that it is supporting MOND, simply look what it has to say about the
Baryonic TFR. This is simply replacing the
luminosity with
total detected baryonic mass in the plot. The small galaxies in this study are gas-dominated. Any error in the assumed stellar mass function is only a small part of a small part, and therefore is too small to affect the conclusion either way.
Quotes:
The BTFR appears to be the
fundamental physical relation underpinning the empiri-
cal Tully-Fisher relation.
...
essentially all of the scatter can be accounted for
by observational uncertainty and the expected variation
in stellar mass-to-light ratios
The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND
http://arxiv.org/abs/1107.2934
SO it seems to be established that the rotation speed is
tightly correlated with the baryonic mass, over many orders of magnitude of galaxy mass.
So back to the Bullet Cluster. This is held up as an example of baryonic and non-baryonic matter
becoming separated. But if this is possible, how come the BTFR has so little (if any) intrinsic scatter? This point alone makes me think non-baryonic matter is not reasonable.