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pro vyhledávání: '"Jmailova, Anna"'
We make use of recent estimates for the parameters of the Milky Way's halo globular clusters and study the influence of the galactic bar on the dynamics of these clusters by computing their orbits. We use both an axisymmetric and non-axisymmetric gal
Externí odkaz:
http://arxiv.org/abs/2303.05603
