Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-14T07:49:49.888Z Has data issue: false hasContentIssue false

The Dynamics Of Galactic Globular Cluster

Published online by Cambridge University Press:  01 April 2008

Chen Ding*
Affiliation:
National Time Service Center, Chinese Academy of Science. Xi'an 710600, China email: ding@ntsc.ac.cn
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have used the Hubble Space Telescope (HST) to measure proper motion of the globular cluster NGC 6656 (M22) with respect to the background bulge stars and its internal velocity dispersion profile. With the space velocity of (Π, Θ, W) = (184±3, 209±14, 132±15) km s−1, we also calculate the orbit of the cluster. The central velocity dispersion in both components of the proper motion of cluster stars is 16.99 km s−1. We derive the mass-to-ration (M/L)∼1.7 which is relatively higher than the past works.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Anderson, J. & King, I. R. 2003 Publication of the Astronomical Society of the Pacific 115, 113CrossRefGoogle Scholar
Trager, S. C., Djorgovski, S., & King, I. R., 1993 Structure and Dynamics of globular clusters, ed. Djorgovski, S G and Meylan, G (San Francisco: ASP) 347Google Scholar
Richter, P, Hilker, M., & Richtler, T., 1999 Astron. Astrophys. 350, 476Google Scholar
Zinn, R. 1985 Astrophys. J. 293, 424CrossRefGoogle Scholar
Peterson, R. C. & Cudworth, K. M. 1994 Astrophys. J. 420, 612CrossRefGoogle Scholar
Dinescu, D. I., Girard, T. M., & van Altena, W. F., 1999 Astron. J. 117, 1792CrossRefGoogle Scholar
Allen, C. & Santillan, A., 1991 Rev. Mexicana. Astron. Astrof. 22, 255Google Scholar
Drukier, G. A., Bailyn, C. D., van Altena, W. F., & Girard, T. M. 2003 Astron. J. 125, 2559CrossRefGoogle Scholar
Peterson, C. J. & King, I. R., 1975 Astron. J. 80, 427CrossRefGoogle Scholar