The orbits of 48 globular clusters in a Milky-Way-Like Barred Galaxy
arXiv:astro-ph/0609357 · doi:10.1086/508676
Abstract
The effect of a barred potential (such as the one of the Milky Way) on the galactic orbits of forty-eight globular clusters for which absolute proper motions are known is studied. The orbital characteristics are compared with those obtained for the case of an axisymmetric galactic potential. Tidal radii are computed and discussed for both the better known axisymmetric case and that including a bar. The destruction rates due to bulge and disk shocking are calculated and compared in both galactic potentials.
Accepted for publication in ApJ. 36 pages, 12 figures
Cited by in corpus (27)
- The orbits of open clusters in the Galaxy
- Halo globular clusters observed with AAOmega: dark matter content, metallicity and tidal heating
- Space Velocities of Southern Globular Clusters. V. A Low Galactic Latitude Sample
- N-body Models of Rotating Globular Clusters
- The global mass functions of 35 Galactic globular clusters: I. Observational data and correlations with cluster parameters
- The Outer Envelopes of Globular Clusters. II. NGC 1851, NGC 5824 and NGC 1261
- First evidence of fully spatially mixed first and second generations in globular clusters: the case of NGC 6362
- Evolution of the local spiral structure of the Milky Way revealed by open clusters
- The eye of Gaia on globular clusters structure: tidal tails
- High mass-to-light ratios of UCDs - Evidence for dark matter ?
- The origin and orbit of the old, metal-rich, open cluster NGC 6791: Insights from kinematics
- Six New Galactic Orbits of Globular Clusters in a Milky-Way-Like Galaxy
- Absolute proper motion of the Galactic open cluster M67
- Chemical abundances in the globular clusters NGC 5024 and NGC 5466 from optical and infrared spectroscopy
- The rate of stellar encounters along a migrating orbit of the Sun
- Monte Carlo simulations of multiple populations in globular clusters: constraints on the cooling flow vs. accretion scenario using million bodies simulations
- Treatment of realistic tidal field in Monte Carlo simulations of star clusters
- Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski~2)
- Galactic Orbits of Globular Clusters in the Region of the Galactic Bulge
- Statistical Analysis of the Probability of Interaction of Globular Clusters with Each Other and with the Galactic Center on the Cosmological Time Scale According to Gaia DR2 Data
- Detailed analysis of the variable star population in the globular cluster NGC 7006
- Far-ultraviolet investigation into the galactic globular cluster M30 (NGC 7099): I. Photometry and radial distributions
- Kinematic characteristics of the Milky Way globular clusters based on Gaia DR2 data
- The Axial Zone of Avoidance in the Globular Cluster System and the Distance to the Galactic Center
- Halo Wide Binaries and Moving Clusters as probes of the Dynamical and Merger History of our Galaxy
- Milky Way Globular Clusters: close encounter rates with each other and with the Central Supermassive Black Hole
- Variable stars in Palomar 13; an evaporating globular cluster