Constraints on the Self-Interaction Cross Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657–56
We compare recent results from X-ray, strong lensing, weak lensing, and optical observations with numerical simulations of the merging galaxy cluster 1E 0657-56. X-ray observations reveal a bullet-like subcluster with a prominent bow shock, which gives an estimate for the merger velocity of 4700 km...
Saved in:
Published in | The Astrophysical journal Vol. 679; no. 2; pp. 1173 - 1180 |
---|---|
Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
Chicago, IL
IOP Publishing
01.06.2008
University of Chicago Press |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!