Kinematic characteristics of the Milky Way globular clusters based on Gaia DR2 data
Chemerynska, I. V.; Ishchenko, M. V.; Sobolenko, M. O.; Khoperskov, S. A.; Berczik, P. P.
Ukraine, France, Kazakhstan, Germany, Hungary
Abstract
Using the data from Gaia (ESA) Data Release 2 we performed the orbital calculations of globular clusters (GCs) of the Milky Way. To explore possible close encounters (or collisions) between the GCs, using our own developed high-order φ-GRAPE code, we integrated backward and forward orbits of 119 objects with reliable positions and proper motions. In the calculations, we adopted a realistic axisymmetric Galactic potential (bulge + disk + halo). Using different impact conditions, we found four pairs of six GCs that may have experienced an encounter within twice the sum of the half-mass radii ('collisions') over the last 5 Gyr: Terzan 3 — NGC 6553, Terzan 3 — NGC 6218, Liller 1 — NGC 6522 and Djorg 2 — NGC 6553.