Galactic orbits of globular clusters in the region of the Galactic bulge


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Galactic orbits have been constructed over long time intervals for ten globular clusters located near the Galactic center. A model with an axially symmetric gravitational potential for the Galaxy was initially applied, after which a non-axially symmetric potential corresponding to the central bar was added. Variations in the trajectories of all these globular clusters in the XY plane due to the influence of the bar were detected. These were greatest for the cluster Terzan 4 in the meridional (RZ) plane. The globular clusters Terzan 1, Terzan 2, Terzan 4, Terzan 9, NGC 6522, and NGC 6558 always remained within the Galactic bulge, no farther than 4 kpc from the Galactic center.

作者简介

V. Bobylev

Central (Pulkovo) Astronomical Observatory

编辑信件的主要联系方式.
Email: vbobylev@gao.spb.ru
俄罗斯联邦, Pulkovskoe shosse 65, St. Petersburg, 196140

A. Bajkova

Central (Pulkovo) Astronomical Observatory

Email: vbobylev@gao.spb.ru
俄罗斯联邦, Pulkovskoe shosse 65, St. Petersburg, 196140

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