Globular clusters: absolute proper motions and Galactic orbits

Abstract

We cross-match objects from several different astronomical catalogs to determine the absolute proper proper motions of stars within the 30-arcmin radius fields of 115 Milky-Way globular clusters with the accuracy of 1--2~mas/yr. The proper motions are based on positional data recovered from the USNO-B1, 2MASS, URAT1, ALLWISE, UCAC5, and GAIA DR1 surveys with up to 10 positions spanning an epoch difference of up to $\sim$~65~years, and reduced to GAIA DR1 TGAS frame using UCAC5 as the reference catalog. Cluster members are photometrically identified by selecting horizontal- and red-giant branch stars on color-magnitude diagrams, and the mean absolute proper motions of the clusters with a typical formal error of $\sim$~0.4~mas/yr are computed by averaging the proper motions of selected members. The inferred absolute proper motions of clusters are combined with available radial-velocity data and heliocentric distance estimates to compute the cluster orbits in terms of the Galactic potential models based on Miyamoto and Nagai disk, Hernquist spheroid, and modified isothermal dark-matter halo (axisymmetric model without a bar) and the same model + rotating Ferre's bar (non-axisymmetric). Five distant clusters have higher-than-escape velocities, most likely due to large errors of computed transversal velocities, whereas the computed orbits of all other clusters remain bound to the Galaxy. Unlike previously published results, we find the bar to affect substantially the orbits of most of the clusters, even those at large Galactocentric distances, bringing appreciable chaotization, especially in the portions of the orbits close to the Galactic center, and stretching out the orbits of some of the thick-disk clusters.

arXiv comment14 pages, 14 figures, 3 tables, to appear in Astrophysical Bulletin. Table 1 replaced by corrected version (Tables 2 and 3 are based on correct data and remain unchanged)

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• A comprehensive study of 94 open clusters based on the data from IPHAS, GAIA DR2, and other sky surveys
• Chemical abundances in the metal-intermediate GC NGC 6723
• Comparing bulge RR Lyrae stars with bulge giants -- Insight from 3D kinematics
• The Influence of the Galactic Bar on the Dynamics of Globular Clusters
• Infrared photometry and CaT spectroscopy of globular cluster M 28 (NGC 6626)
• Kinematics of outer halo globular clusters: M 75 and NGC 6426
• Globular Clusters of the Galaxy: Chemical Composition vs Kinematics
• Inconsistency of Chemical Properties of Stellar Populations in the Thick Disk Subsystem of Our Galaxy
• Very metal-poor stars in the solar vicinity: kinematics and abundance analysis