Peter,
Thanks again for your reply, which was to some extent helpful in identifying the source of confusion. However, I must point out that you've not addressed the specific reference to the image caption referring to "Visible 'Dark Matter'. Galaxy Cluster CL 0024+17." As demonstrated by the NASA & Wikipedia references, this is definitely a misinterpretation.
Your last response stated:
"Just to give you a flavour, a Sept AGN paper abstract is here, discussing the high density jets of re-ionized matter. And one thing I forgot the Milky Way certainly DOES 'still have' and AGN. (iro Sagattarius A) Not (back) up to any great speed yet, so the 14 hypervelocity stars it has spat out recently are still in one piece, but there's also plenty of ions and gas."
The Milky Way certainly does NOT exhibit the relativistic jets characteristic of an AGN. As I understand, the enormous gamma-ray emitting polar bubbles of plasma are thought to be the remnants of past galaxy nucleus activity. Please see the NASA press release, NASA'S Fermi Telescope Discovers Giant Structure In Our Galaxy.
Your Claude-André Faucher-Giguère, Eliot Quataert reference abstract makes no mention of dark matter. I could not find a free version of that paper, however, I think much more to the point, an FQXi essay entry attributes the observed rotational velocity of spiral galaxies to those very same AGN outflows producing spiral arms moving to the galaxy periphery. This proposal also does not require dark matter to explain the observed rotational characteristics of spiral galaxies. Please see A New Model Without Dark Matter for the Rotation of Spiral Galaxies: The Connections Among Shape, Kinematics and Evolution by Mario Everaldo de Souza.
Still trying to understand the source of confusion regarding visible dark matter, I could not find any accessable Claude-André Faucher-Giguère papers in arXiv, but I did find some with contributor Eliot Quataert. Specifically, I found a very curious report, On the Structure of Hot Gas in Halos: Implications for the Lx-Tx Relation & Missing Baryons. As the title implies this model evaluation of, as I understand, hot gases in the intraclustr medium of galaxy clusters is also applied to the composition of galaxy dark matter halos. It also suggests that galaxies were formed from primordial dark matter.
What I think may be occurring is that researchers studying the characteristics of hot gaseous intracluster media (ICM) (perhaps produced by AGN outflows) are applying their results to supposedly galactic dark matter halos thought to have been accreted from the hot gas/presumptive dark matter ICM, depleted of baryonic gases.
I can understand how confusing this is from the varying perspective of those studying hot gases in the ICM and the presumedly colocated galaxy cluster dark matter, and those that specified the presence of dark matter to explain the non-Keplerian rotational characteristics of spiral galaxies.
Keep in mind that the visible ICM matter is thought to be twice as massive as the visible galactic matter of all galaxies within a galaxy cluster. It's difficult to understand how the more massive visible ICM could have been ejected from the relativistic jets of less massive AGN.
Moreover, galactic dark matter halos are thought to be about 10x the visible mass of spiral galaxies - this mass seeming to be necessary. It's also very difficult to believe that AGNs produce much more massive dark matter galactic halos.
At any rate, I have yet to see any reference to "visible 'dark matter'" in galactic halos. I don't think there's any support for this interpretation in any of the literature.
I hope this helps, Jim