Hostname: page-component-7479d7b7d-wxhwt Total loading time: 0 Render date: 2024-07-12T19:35:52.457Z Has data issue: false hasContentIssue false
  • English
  • Français

Dynamical Friction in the Coma Cluster

Published online by Cambridge University Press:  14 August 2015

M. Lecar
M. Lecar*
Affiliation:
Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Mass., U.S.A.

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.

If the galaxies composing the Coma Cluster were initially ‘Ostriker-Peebles’ galaxies (i.e., isothermal spheres extending to 250–500 kpc), the hidden mass is likely to be tidally torn-off halos. Owing to dynamical friction, the remnant cores tend to spiral in to the center of the cluster. This happens as long as the hidden mass, whatever its origin, consists of objects much less massive than galaxies.

Type
Part I/Spherical Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 161 - 166
Copyright
Copyright © Reidel 1975 

References

Alladin, S. M.: 1965, Astrophys. J. 141, 768.CrossRefGoogle Scholar
Alladin, S. M., Sastry, K. S., and Ballabh, G. M.: 1974, in Barbanis, B. and Hadjidemetriou, J. (eds.), Galaxies and relativistic Astrophysics, Springer-Verlag, Berlin, p. 129.CrossRefGoogle Scholar
Alladin, S. M., Potdar, A., and Sastry, K. S.: 1974, this volume, p. 167.CrossRefGoogle Scholar
Bahcall, N. A.: 1973, Astrophys. J. 183, 783.CrossRefGoogle Scholar
Bardeen, J. M.: 1974, this volume, p. 297.CrossRefGoogle Scholar
Biermann, P.: 1974, ‘Report to the Faculty of Mathematical Sciences’, George August University, Gottingen.Google Scholar
Chandrasekhar, S. and Wares, G. W.: 1949, Astrophys. J. 109, 551.CrossRefGoogle Scholar
Gallagher, J. S. III and Ostriker, J. P.: 1972, Astron. J. 77, 288.CrossRefGoogle Scholar
Hénon, M.: 1973, in Martinet, L. and Mayor, M. (eds.), Dynamical Structure and Evolution of Stellar Systems, Geneva Observatory, p. 214.Google Scholar
Lauberts, A.: 1974, Astron. Astrophys. 33, 231.Google Scholar
Oemler, A. Jr.: 1973, ‘The Systematic Properties of Clusters of Galaxies’, California Institute of Technology ().Google Scholar
Omer, G. C. Jr., Page, T. L., and Wilson, A. G.: 1965, Astron. J. 70, 440.CrossRefGoogle Scholar
Ostriker, J. P. and Peebles, P. J. E.: 1973, Astrophys. J. 186, 467.CrossRefGoogle Scholar
Peebles, P. J. E.: 1970, Astron. J. 75, 13.CrossRefGoogle Scholar
Roberts, M. S.: this volume, p. 331.Google Scholar
Rood, H. J., Page, T. L., Kintner, E. C., and King, I. R.: 1972, Astrophys. J. 175, 627.CrossRefGoogle Scholar
Saslaw, W. C. and de Young, D. S.: 1971, Astrophys. J. 170, 423.CrossRefGoogle Scholar
Sastry, K. S. and Alladin, S. M.: 1970, Astrophys. Space Sci. 9, 261.CrossRefGoogle Scholar
Spitzer, L. Jr.: 1969, Astrophys. J. 158, L139.CrossRefGoogle Scholar