Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-30T00:38:28.906Z Has data issue: false hasContentIssue false
  • English
  • Français

Relativistic Stellar Dynamics

Published online by Cambridge University Press:  04 August 2017

G. Contopoulos
G. Contopoulos*
Affiliation:
University of Athens, Greece

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.

Three main areas of relativistic stellar dynamics are reviewed: (a) Relativistic clusters, (b) Systems containing a massive black hole, and (c) Perturbed expanding Universes. The emphasis is on the use of orbit perturbations.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 417 - 423
Copyright
Copyright © Reidel 1983 

References

Bardeen, J.M., Press, W.H. and Teukolsky, S.A.: 1972, Astrophys J. 178, p. 347.Google Scholar
Carter, B.: 1968, Phys. Rev. 174, p. 1559.Google Scholar
Chandrasekhar, S.: 1982, “The Mathematical Theory of Black Holes” (in press).Google Scholar
Contopoulos, G.: 1960, Z. Astrophys. 49, p. 273.Google Scholar
Contopoulos, G.: 1982, preprint.Google Scholar
Friedmann, J.L.: 1978, Commun. Math. Phys. 62, p. 247.Google Scholar
Friedmann, J.L. and Shutz, B.F., 1978, Astrophys. J. 222, p. 281.Google Scholar
Ipser, J.P.: 1975, IAU Symposium 69, p. 423.Google Scholar
Lynden-Bell, D. and Wood, R.: 1968, Monthly Notices Roy. Astron. Soc. 138, p. 495.Google Scholar
Penrose, R.: 1969, Riv. Nuovo Cimento 1, p. 252.Google Scholar
Sharp, N.A.: 1979, Gen. Rel. Gravitation 10, p. 659.CrossRefGoogle Scholar
Spyrou, N. and Varvoglis, H.: 1982, Astrophys. J. 255, p. 674.Google Scholar
Vandervoort, P.O. and Ipser, J.R.: 1982, Astrophys. J. 256, p. 497.Google Scholar