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Beyond IDCS J1426.5+3508
On Wednesday, October 3, 2012 9:58:43 AM UTC+2, Phillip Helbig
wrote: Why do you expect the density to be as you described it? I expect that a galaxy cluster more or less is the same as a dwarf eliptical galaxy like: NGC 147 See: http://en.wikipedia.org/wiki/NGC147 That means the highest density is in the center and slowly decreases. Those distributions are the same I have used to study the Virial Theorem This description is identical for the bulge of our Milky Way. The following link is "interesting": http://en.wikipedia.org/wiki/Virial_...#Virial_radius They use the equation rho c = 3*H^2/8*pi*G to study the behaviour of a single galaxy cluster while at the same type that same equation is used to study the whole Universe. Nicolaas Vroom http://users.telenet.be/nicvroom |
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