ИСТИНА

High energy and cold plasma streams and gas/dust flows in the interstellar medium (ISM) form the net spatiotemporal structure of the Universe. Cloud-cloud collisions (CCC) between molecular clouds (MCs) and interplay of the last with strong shock wave of remnants after supernova explosion are proposed as key mechanisms for triggering protostars originated in highly compression zones of new formations. The paper is devoted to study consequences of supersonic turbulization of MCs matter in numerical simulation following different scenarios of shock interplay and key instabilities influence onto emergent dense clumps and filamentous structures originated here. To simulate a fine structure of shock colliding flows authorized Eulerian code with parallelization on high resolution mesh with more two billions nodes was performed.