Dynamical Evolution of M92 Globular Cluster - Proving the Milky-Way Disk-Shocking

Details Dynamical Evolution of M92 Globular Cluster - Proving the Milky-Way Disk-Shocking Dynamical Evolution of M92 Globular Cluster - Proving the Milky-Way Disk-Shocking

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..275..444d&link_type=abstract

Disks of Galaxies: Kinematics, Dynamics and Peturbations, ASP Conference Proceedings, Vol. 275. Edited by E. Athanassoula, A. Bo

Astronomy and Astrophysics

Astronomy

Scientific paper

Treecode N-body numerical simulations are used to study the dynamical
evolution of the globular cluster M92 in the Galaxy gravitational field
during the last two Gyr, which corresponds to approximately 16
perigalactic transits.

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