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Passing through the Galactic disk, a massive object such as a globularcluster, can trigger star formation process leading to the birth of openclusters. Here, we analyze such possible evolutionary relationship betweenglobular and open clusters. To search for the closest rapprochement betweenobjects we computed backwards the orbits of 150 Galactic globular and 232 openclusters (younger than 100 Myr) with proper motions, derived from the Gaia DR2Catalog. The orbits were computed using the recently modified three-component(disk, bulge and halo) axisymmetric Navarro-Frenk-White potential, which wascomplemented by non-axisymmetric bar and spiral density wave potentials. Weobtained a new estimate for the frequency of impacts of globular clusters aboutthe Galactic disk, which is equal to 4 events for 1 million years. In theframework of the considered scenario, we highlight the following nine pairs ofglobular and open clusters, with rapprochement within 1 kpc at the time of theintersection the Galactic disk by a globular cluster for the latest 100 Myr:  NGC 104 - Turner 3,  NGC 104 - NGC 6396,  NGC 104 - Ruprecht 127,  NGC 5139 - Trumpler 17,  NGC 5139 - NGC 6520,  NGC 6341 - NGC 6613,  NGC 6838 - NGC 6520,  NGC 7078 - NGC 7063,  NGC 6760 - Ruprecht 127.

Search for the evolutionary relationship between Galactic globular and open clusters using data from the Gaia DR2 Catalog