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In this work we are interested to study the by-products of SNR-clouds in astarburst (SB) system. These interactions can have an important role in therecycling of matter from the clouds to the ISM and vice-versa. In the presentwork, we have focused our attention on the global effects of the interactionsbetween clouds and SN shock waves in the ISM of SB environments, and performed3-D radiative cooling hydrodynamical simulations with the adaptive YGUAZU gridcode. We have also considered the effects of the photo-evaporation due to thepresence of a high number of UV photons from hot stars and supernovae (SNe).The results have shown that, in the presence of radiative cooling, instead ofan efficient gas mixing with the diffuse ISM, the interactions cause thefragmentation of the clouds into smaller ones. The results have also revealedthat the SNR-clouds interactions are less efficient at producing substantialmass loss from the clouds to the diffuse ISM than mechanisms such as thephoto-evaporation caused by the UV flux from the hot stars.

Multidimensional hydrodynamical simulations of radiative cooling SNRs-clouds interactions: an application to starburst environments