Dynamical Modeling of M13 Proper Motions

  • Kyle Cudworth
  • D. N. C. Lin
  • Kap-Soo Oh
Chapter
Part of the International Astronomical Union. Symposium book series (IAUS, volume 113)

Abstract

Proper motion data of Ml3 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.

Keywords

Velocity Dispersion Proper Motion Cluster Member Cluster Star Sloan Foundation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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Reference

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

Copyright information

© International Astronomical Union 1985

Authors and Affiliations

  • Kyle Cudworth
    • 1
  • D. N. C. Lin
    • 2
  • Kap-Soo Oh
    • 2
  1. 1.Yerkes ObservatoryUniversity of ChicagoUSA
  2. 2.Lick ObservatoryUniversity of CaliforniaSanta CruzUSA

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