Chemerynska, I. V. and Ishchenko, M. V. and Sobolenko, M. O. and Khoperskov, S. A. and Berczik, Péter (2022) Kinematic characteristics of the Milky Way globular clusters based on Gaia DR-2 data. ADVANCES IN ASTRONOMY AND SPACE PHYSICS. ISSN 2227-1481
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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 phi-GRAPE code, we integrated (backward and forward) the orbits of 119 objects with reliable positions and proper motions. In calculations, we adopted a realistic axisymmetric Galactic potential (bulge + disk + halo). Using different impact conditions, we found four pairs of the six GCs that may have experienced an encounter within twice the sum of the half-mass radii (collisions) over the last 5Gyr: Terzan3 - NGC 6553, Terzan 3 - NGC 6218, Liller 1 - NGC 6522 and Djorg 2 - NGC 6553.
Item Type: | Article |
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Uncontrolled Keywords: | Astrophysics - Astrophysics of Galaxies; |
Subjects: | Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika Q Science / természettudomány > QC Physics / fizika |
SWORD Depositor: | MTMT SWORD |
Depositing User: | MTMT SWORD |
Date Deposited: | 14 Nov 2022 09:00 |
Last Modified: | 14 Nov 2022 09:00 |
URI: | http://real.mtak.hu/id/eprint/153439 |
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