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Dynamical Modeling of M13 Proper Motions

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Dynamics of Star Clusters

Part of the book series: International Astronomical Union. Symposium ((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.

Alfred P. Sloan Foundation Fellow

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Author information

Authors and Affiliations

  1. Yerkes Observatory, University of Chicago, USA

    Kyle Cudworth

  2. Lick Observatory, University of California, Santa Cruz, USA

    D. N. C. Lin & Kap-Soo Oh

Authors
  1. Kyle Cudworth
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  2. D. N. C. Lin
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  3. Kap-Soo Oh
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Editor information

Editors and Affiliations

  1. California Institute of Technology, Pasadena, California, USA

    Jeremy Goodman

  2. The Institute for Advanced Study, Princeton, New Jersey, USA

    Piet Hut

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© 1985 International Astronomical Union

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Cudworth, K., Lin, D.N.C., Oh, KS. (1985). Dynamical Modeling of M13 Proper Motions. In: Goodman, J., Hut, P. (eds) Dynamics of Star Clusters. International Astronomical Union. Symposium, vol 113. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5335-2_6

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  • DOI: https://doi.org/10.1007/978-94-009-5335-2_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-277-1965-2

  • Online ISBN: 978-94-009-5335-2

  • eBook Packages: Springer Book Archive

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