  Passing through the Galactic disk, a massive object such as a globular
cluster, can trigger star formation process leading to the birth of open
clusters. Here, we analyze such possible evolutionary relationship between
globular and open clusters. To search for the closest rapprochement between
objects we computed backwards the orbits of 150 Galactic globular and 232 open
clusters (younger than 100 Myr) with proper motions, derived from the Gaia DR2
Catalog. The orbits were computed using the recently modified three-component
(disk, bulge and halo) axisymmetric Navarro-Frenk-White potential, which was
complemented by non-axisymmetric bar and spiral density wave potentials. We
obtained a new estimate for the frequency of impacts of globular clusters about
the Galactic disk, which is equal to 4 events for 1 million years. In the
framework of the considered scenario, we highlight the following nine pairs of
globular and open clusters, with rapprochement within 1 kpc at the time of the
intersection 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.
