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L. A. Phillips, J. P. Ostriker (Princeton U.), M. J. Freyberg, J. Tümper (MPE)
We present simulations of the Warm/Hot gas contribution to the soft X-ray background. The expected gas autocorrelation function, gas/galaxy cross-correlation function and hardness ratios are calculated from the simulations and compared to observations. We discuss the contribution of the Warm/Hot gas component to the soft X-ray background in ROSAT All-Sky Survey maps.