However, in your review of the early parts of this thread - I think you said you'd be undertaking such a review, right? - please pay attention to Z's posting style. ...
I have looked at the earlier posts, though I admit in a less than completely rigorous fashion. I think I have seen enough of everyone's posts, here and on other boards, to get the point.
The flaw in this argument is this assumption that all the ordinary matter in galaxies is in easily-visible, bright, stars. Instead, most of the mass of galaxies may well be in the form of dwarf stars, which produce very little light per unit mass, in other words have a very high mass-to-light ratio. Several studies of galaxies using very long exposures have shown that they have 'red halos', halos of stars that are mostly red dwarfs. Other studies have indicated that the halos may be filled with white dwarfs, the dead remains of burnt-out stars. In addition, there is evidence that a huge amount of mass may be tied up in relatively cool clouds of plasma that do not radiate much x-ray radiation, and would be in closer proximity to the galaxies than the hot plasma.
This turns out not to be much of an argument, and is in fact one that has already been addressed in the literature. It is, therefore, not an "assumption" at all, in the sense you mean, but rather a logical consequence of observation.
First, let me address the case of the Milky Way in particular. We can't see it from outside, but of course we are a lot closer to the stellar halo of our own Galaxy than we are to the halo of any other galaxy. The advent of the Hubble Space Telescope has made it possible to search for read dwarf stars directly in the Milky Way halo, which could not be previously done from the ground. The result is that there are far too few red dwarf stars in the Galactic halo to account for the gravitational requirements that lead to the assumption of dark matter (see, i.e.
Hubble Rules Out a Leading Explanation for Dark Matter, press release & images dated 17 October 1994). And see the paper
The stellar halo of the Galaxy; Amina Helmi, The Astronomy and Astrophysics Review 15(3): 145-188, June 2008. This paper reviews the stellar halo of the Milky Way in detail, and includes a comment on gravitational microlensing that is relevant & important:
For example, if a significant fraction of the dark matter had been baryonic (composed by MACHO's,
Paczynski 1986), then the stellar and dark halos would presumably be indistinguishable. However, this scenario appears unlikely, as the microlensing surveys are unable to assign more than 8% of the matter to compact dark objects (
Tisserand et al. 2007, although see
Alcock et al. 2000 for a different, though earlier result).
The "different though earlier" result from Alcock,
et al., 2007 puts the halo MACHO fraction at 20%, and estimates the total MACHO mass of the halo at about 9x10
10 solar masses. Compare this to a total Milky Way mass of a few times 10
12 solar masses, and we see that even with the most optimistic assumptions, the total MACHO mass of the Milky Way halo is no more than about 10% of the total mass of the Galaxy. Hence, for the case of our own Milky Way, the assumption of non baryonic dark matter cannot be avoided, assuming the baryons come in the form of compact objects. I will have more to say about that shortly.
Now, let us consider the red halos that Zeuzzz refers to, supporting his claim that these halos could represent most or all of the dark matter as baryonic mass. To begin with, note the result already established above for our own Milky Way. If we make the not so bold assumption that the Milky Way is not a special case as spiral galaxies go, then we would expect that the same should be true for other spiral galaxies, on average. Namely, they do not have significant baryonic halos in the form of compact objects. This already makes the assumption that this is indeed the case for the
Bullet Cluster galaxies a reasonable one. However, see the paper
Red Halos of Galaxies Reservoirs of Baryonic Dark Matter?, Zackrisson
et al., May 2008, from the IAU symposium proceedings. The red halos are not just "faint", they are "extremely faint".
Zibetti, White & Brinkman, 2004 had to stack scaled images of 1047 galaxies from the SDSS just to get reliable photometry for halos with surface brightness of about 30 magnitudes per square arcsecond. The multiband colors for their stacked halo look like the color of the halo found around NGC 5907. However,
Yost et al., 2000 looked at NGC 5907 in the near infrared, 3.5 - 5 microns, and did not detect the halo at all. These observations pose significant problems for interpretation. The multiband colors are not consistent with a normal distribution of stellar masses, and require a population unusually rich in low mass stars. However, low mass stars should stand out well in the near infrared, so a literal interpretation of the failure to detect the halo of NGC 5907 in the near infrared would imply that the halo is not made of stars at all. In any case, that failure limits the baryonic mass fraction of the halo to about 15%, if it is in fact made up of red dwarf stars.
The upshot of all this is that observation places strong limits on the mass available in these red halos. Photometry, sensitive to red dwarf stars, and microlensing, sensitive to all compact objects, both clearly show that there is not enough mass in the halo to account for the mass required to explain the dark matter effect. And the difference is significant. So there is no "flaw in the assumption" of Clowe et al., so long as we are talking about compact objects.
As for the gas clouds, they too will not do the job. In a collision between galaxies, we expect individual stars to collide only rarely, if at all. Likewise, in a collision between galaxy clusters, we expect individual galaxies to collide only rarely. However, the intracluster gas should undergo significant collision, as shown in the Clowe et al. paper. If there are cold intracluster clouds, they will be heated by the collision and emit X-rays. Only small clouds tied to the galaxy might escape this fate. But those clouds must carry negligible mass. After all,
Briggs, 2004 tells us "
Neutral intergalactic clouds are so greatly out numbered by galaxies that their integral HI content is negligible in comparison to that contained in optically luminous galaxies." HI is neutral hydrogen. So here again, observation clearly implies that the dark matter cannot be made of HI clouds.
So the conclusion is that the argument put forward by
Zeuzzz is not valid. The "flaw in the assumption" is imaginary and not real. The conclusion reached by
Clowe et al. stands at least as a reasonable interpretation of the observations. However, as we see from the 193 citations (so far), there is considerable discussion of the interpretation of the Bullet Cluster collision. There are claims that modified gravity theories can still do away with dark matter, and explain the observations, but this remains controversial. This is a point worth noting. There are legitimate alternative explanations put forth for discussion, based on modified gravity theories. They are not conclusive, but they are scientifically valid exercises. However,
Zeuzzz, and other alternative critics typical of this and other discussion groups, are far to dismissive and arrogant in their approach, and base their claims not on legitimate scientific grounds, but on simplistic knee-jerk reactions. Just a little research would have quickly shown the the alternative put forth by
Zeuzzz has already been outdated by research that is in some cases many years old.