13 enero 2015
Researchers have revealed that considering environmental effects such as a gravitational tidal force spread over a scale much larger than a galaxy cluster is indispensable to explain the distribution and evolution of dark matter halos around galaxies. A detailed comparison between theory and simulations made this work possible.
http://feeds.sciencedaily.com/~r/sciencedaily/~3/OANiHPvWttw/150113111535.htm
