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Dynamical Evolution of Globular Clusters After Core Collapse

Published online by Cambridge University Press:  04 August 2017

Douglas C. Heggie
Douglas C. Heggie*
Affiliation:
University of Edinburgh, Department of Mathematics, King's Buildings. Edinburgh EH9 3JZ, U.K.

Abstract

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This review describes work on the evolution of a stellar system during the phase which starts at the end of core collapse. It begins with an account of the models of Hénon, Goodman, and Inagaki and Lynden-Bell, as well as evaporative models, and modifications to these models which are needed in the core. Next, these models are related to more detailed numerical calculations of gaseous models, Fokker-Planck models, N-body calculations, etc., and some problems for further work in these directions are outlined. The review concludes with a discussion of the relation between theoretical models and observations of the surface density profiles and statistics of actual globular clusters.

Type
Dynamical Evolution of Globular Clusters
Information
Symposium - International Astronomical Union , Volume 113: Dynamic of Stars Clusters , 1985 , pp. 139 - 160
Copyright
Copyright © Reidel 1985 

References

Alexander, M.E. & Budding, E.: 1979, Astron. Astrophys. 73, 227.Google Scholar
Bettwieser, E. & Fritze, U.: 1984, submitted to P.A.S.J. Google Scholar
Bettwieser, E. & Inagaki, S.: 1984, ‘A Gas Model for Multi-Component Star Clusters: 1. Method and Comparison with Fokker-Planck,’ in preparation.Google Scholar
Bettwieser, E. & Sugimoto, D.: 1984, M.N.R.A.S., in press.Google Scholar
Cohn, H.: 1980, Ap. J. 242, 765.Google Scholar
Cohn, H. & Hut, P.: 1984, Ap. J. Lett. 277, L45.Google Scholar
Djorgovski, S. & King, I.R.: 1984, Ap. J. Lett. 277, L49.CrossRefGoogle Scholar
Dokuchaev, V.I. & Ozernoy, L.M.: 1982, Astron. Astrophys. 111, 16.Google Scholar
Duncan, M.J. & Shapiro, S.L.: 1982, Ap. J. 253, 921.Google Scholar
Fall, S.M. & Malkan, M.A.: 1978, M.N.R.A.S. 185, 899.Google Scholar
Goodman, J.: 1984, Ap. J. 280, 298.Google Scholar
Hachisu, I., Nakada, Y., Nomoto, L. & Sugimoto, D.: 1978, Prog. Theor. Phys. 60, 393.Google Scholar
Heggie, D.C.: 1980, in Hesser, J. E. (ed.), Star Clusters, Reidel, Dordrecht, p. 401.Google Scholar
Heggie, D.C.: 1984, M.N.R.A.S. 206, 179.CrossRefGoogle Scholar
Hénon, M.: 1961, Ann. d'Astrophys. 24, 369.Google Scholar
Hénon, M.: 1965, Ann. d'Astrophys. 28, 62.Google Scholar
Hénon, M.: 1975, in Hayli, A. (ed.), Dynamics of Stellar Systems, Reidel, Dordrecht, p. 133.Google Scholar
Hills, J.G.: 1975, Astron. J. 80, 1075.Google Scholar
Illingworth, G. & King, I.R.: 1977, Ap. J. Lett. 218, L109–12.Google Scholar
Inagaki, S. & Lynden-Bell, D.: 1983, M.N.R.A.S. 205, 913.Google Scholar
King, I.R.: 1965, Astron. J. 70, 376.Google Scholar
King, I.R.: 1966, Astron. J. 71, 64.Google Scholar
Larson, R.B.: 1970a, M.N.R.A.S. 147, 323.Google Scholar
Larson, R.B.: 1970b, M.N.R.A.S. 150, 93.Google Scholar
Larson, R.B.: 1984, ‘Black-Hole Remnants in Globular Clusters’, preprint.Google Scholar
Lightman, A.P.: 1982, Ap. J. Lett. 263, L19.CrossRefGoogle Scholar
Lightman, A.P., Press, W.H. & Odenwald, S.F.: 1978, Ap. J. 219, 629.Google Scholar
Lightman, A.P. & Shapiro, S.L.: 1978, Rev. Mod. Phys. 50, 437.Google Scholar
Lynden-Bell, D. & Eggleton, P.P.: 1980, M.N.R.A.S. 191, 483.Google Scholar
McMillan, S.L.W. & Lightman, A.P.: 1984a, Ap. J., in press.Google Scholar
McMillan, S.L.W. & Lightman, A.P.: 1984b, Ap. J., in press.Google Scholar
McMillan, S.L.W., Lightman, A.P. & Cohn, H.: 1981, Ap. J. 251, 436.CrossRefGoogle Scholar
Marchant, A.B. & Shapiro, S.L.: 1980, Ap. J. 239, 685.Google Scholar
Ozernoy, L.M. & Dokuchaev, V.I.: 1982, Astron. Astrophys. 111, 1.Google Scholar
Peaterson, C.J. & King, I.R.: 1975, Astron. J. 80, 427.Google Scholar
Retterer, J.M.: 1984, ‘A Dynamical Model for Small Stellar Systems,’ preprint.Google Scholar
Shapiro, S.L.: 1977, Ap. J. 217, 281.Google Scholar
Spitzer, L. Jr. & Shull, J.M.: 1975a, Ap. J. 200, 339.Google Scholar
Spitzer, L. Jr. & Shull, J.M.: 1975b, Ap. J. 201, 773 Google Scholar
Stodóℓkiewicz, J.S.: 1982, Acta Astron. 32, 63.Google Scholar
Stodóℓkiewicz, J.S.: 1983, in Ruprecht, J. & Palouš, J. (eds.), Star Clusters and Associations and their Relation to the Evolution of the Galaxy , Astron. Inst. Czech. Acad. Sci., Prague, p. 103.Google Scholar
von Hoerner, S.: 1960, Z. Astrophys. 50, 184.Google Scholar
von Hoerner, S.: 1963, Z. Astrophys. 57, 47.Google Scholar