A comparison of X-ray and strong lensing properties of simulated X-ray clusters
A comparison of X-ray and strong lensing properties of simulated X-ray clusters
We use gas-dynamical simulations of galaxy clusters to compare their X-ray and strong lensing properties. Special emphasis is laid on mass estimates. The cluster masses range between 6 x 10^14 solar masses and 4 x 10^15 solar masses, and they are examined at redshifts between 1 and 0. We compute …