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They are usually found close to the centers of galaxy clusters.
The number of galaxy clusters that form depends on dark energy in two ways.
They can be found near the centres of some rich galaxy clusters.
The dark energy survey will discover a large number of galaxy clusters.
Galaxy clusters are the largest known structures in the universe.
It is the result of a still ongoing merger between two galaxy clusters.
He has also advanced a new hypothesis on the structure of galaxy clusters.
Where C is a constant which depends on the distance to the galaxy clusters.
It will help to probe the nature of dark energy by finding very distant galaxy clusters.
The survey will measure the abundance and properties of galaxy clusters.
The huge spaces between galaxy clusters are called the voids.
Other methods are based more on the statistics and probabilities of things such as entire galaxy clusters.
The strongest lensing occurred at the galaxy clusters, rather than the gas.
The cluster was formed by four separate galaxy clusters that have been involved in a collision.
Only very large non-bound systems (say, galaxy clusters) expand with the universe.
Two rather smaller galaxy clusters were also unveiled that will help lay out this timeline.
It did not state how to calculate gravitational lensing from galaxy clusters.
A simple application of the virial theorem concerns galaxy clusters.
This model is valid in the present era only on large scales (roughly the scale of galaxy clusters and above).
Apparently, these ripples gave rise to the present vast cosmic web of galaxy clusters and dark matter.
These perturbations were indispensable to the formation of galaxies and galaxy clusters.
An important experimental probe of dark enery comes from counting galaxy clusters.
From gluons to galaxy clusters, all conveniently arrayed in size order.
It occurred 100 million years ago when two galaxy clusters three billion light-years away passed through each other at about 10 million miles an hour.
There are mainly three scenarios for the origin of galaxy clusters and superclusters.
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