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Gaseous Models

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Dynamics of Star Clusters

Part of the book series: International Astronomical Union. Symposium ((IAUS,volume 113))

Abstract

We can understand physics of self-gravitating system in terms of gaseous models in so far that their global natures and effects of self-gravity are concerned. Here summarized what are known in idealized gaseous models. They include gravothermal collapse/expansion in linear and non-linear regimes, and post-collapse evolution with gravothermal oscillation. Also discussed are their relations with discrete system and with treatment in statistical mechanics.

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References

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Author information

Authors and Affiliations

  1. Department of Earth Science and Astronomy, College of Arts and Sciences, University of Tokyo, Japan

    Daiichiro Sugimoto

Authors
  1. Daiichiro Sugimoto
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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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Sugimoto, D. (1985). Gaseous Models. 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_23

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  • DOI: https://doi.org/10.1007/978-94-009-5335-2_23

  • 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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