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Massive young star clusters contain dozens or hundreds of massive stars thatinject mechanical energy in the form of winds and supernova explosions,producing an outflow which expands into their surrounding medium, shocking itand forming structures called superbubbles. The regions of shocked material canhave temperatures in excess of 10$^6$ K, and emit mainly in thermal X-rays(soft and hard). This X-ray emission is strongly affected by the action ofthermal conduction, as well as by the metallicity of the material injected bythe massive stars. We present three-dimensional numerical simulations exploringthese two effects, metallicity of the stellar winds and supernova explosions,as well as thermal conduction.

The soft and hard X-rays thermal emission from star cluster winds with a supernova explosion