Abstract
3D numerical simulations of the Arches cluster wind are presented. In order to make these simulations as close the observations as possible, we have taken the positions (on the plane of the sky) of the 60 brightest stars and we have created three possible 3D spatial distributions. For each of these configurations, we have obtained simulated X-ray maps and spectra, for comparing directly with recent observations of this cluster obtained with the Chandra satellite by Yusef-Zadeh and coworkers.
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