Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-12-04T19:36:38.186Z Has data issue: false hasContentIssue false
  • English
  • Français

Dynamical Modeling of M13 Proper Motions

Published online by Cambridge University Press:  04 August 2017

Kyle Cudworth ,
D.N.C. Lin  and
Kap-Soo Oh
Kyle Cudworth
Affiliation:
Yerkes Observatory University of Chicago
D.N.C. Lin
Affiliation:
Lick Observatory University of California, Santa Cruz
Kap-Soo Oh
Affiliation:
Lick Observatory University of California, Santa Cruz

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.

Proper motion data of M13 cluster members are very useful for the investigation of the cluster's internal dynamics. We introduce a maximum likelihood method to fit these data in terms of conventional King-Michie models.

Type
May 29: Observations of Globular Clusters
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 65 - 67
Copyright
Copyright © Reidel 1985 

References

Cudworth, K.M. and Monet, D.G.: 1979, Astron. J., 84, 774.Google Scholar