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The Collapse and Formation of Galaxies

Published online by Cambridge University Press:  14 August 2015

R. B. Larson
R. B. Larson*
Affiliation:
Yale University Observatory, New Haven, Conn., U.S.A.

Extract

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The ultimate aim of studies of the dynamics of stellar systems is to gain an understanding of why they have the structures that are observed, how they might have formed, and how they might evolve with time. In the case of galaxies, unlike smaller astronomical systems such as stars and star clusters, the problem of understanding their present structure is inseparable from the problem of understanding their formation since, as has long been clear, the two-body relaxation time in galaxies is much longer than the age of the universe, so that properties such as the radial density distribution and the flattening of elliptical galaxies cannot have changed significantly since they were formed. Other features of galaxies, such as the presence of spiral patterns or nuclear activity, may be of a more transitory nature and not closely related to the formation process, but such phenomena probably involve mainly the gas component of galaxies and may be regarded as perturbations on the underlying stellar system, whose basic structure must still be understood in terms of the formation process.

Type
Part II/Flattened Systems
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 247 - 269
Copyright
Copyright © Reidel 1975 

References

Alladin, S. M., Potdar, A., and Sastry, K. S.: 1975, this volume, p. 167.CrossRefGoogle Scholar
Arp, H. C.: 1965, Stars and Stellar Systems 5, 401.Google Scholar
Bardeen, J. M.: 1975, this volume, p. 297.CrossRefGoogle Scholar
Bertola, F. and Capaccioli, M.: 1975, this volume, p. 373.Google Scholar
Binney, J.: 1974, Monthly Notices Roy. Astron. Soc. 168, 73.CrossRefGoogle Scholar
Brosche, P.: 1970, Astron. Astrophys. 6, 240.Google Scholar
Eggen, O. J., Lynden-Bell, D., and Sandage, A. R.: 1962, Astrophys. J. 136, 748.Google Scholar
Faber, S. M.: 1973, Astrophys. J. 179, 731.CrossRefGoogle Scholar
Freeman, K. C.: 1970, Astrophys. J. 160, 811.Google Scholar
Goldreich, P. and Lynden-Bell, D.: 1965, Monthly Notices Roy. Astron. Soc. 130, 125.CrossRefGoogle Scholar
Gott, J. R.: 1973, Astrophys. J. 186, 481.Google Scholar
Gott, J. R.: 1975, Astrophys. J. (in press).Google Scholar
Hartwick, F. D. A. and Sargent, W. L. W.: 1974, Astrophys. J. 190, 283.CrossRefGoogle Scholar
Hohl, F.: 1971, Astrophys. J. 168, 343.Google Scholar
Hohl, F.: 1975, this volume, p. 349.CrossRefGoogle Scholar
Icke, V.: 1973, Astron. Astrophys. 27, 1.Google Scholar
Janes, K. A.: 1975, in press.Google Scholar
King, I. R.: 1966, Astron. J. 71, 64.CrossRefGoogle Scholar
King, I. R.: 1975, in preparation.Google Scholar
Larson, R. B.: 1969, Monthly Notices Roy. Astron. Soc. 145, 405.Google Scholar
Larson, R. B.: 1972a, Nature 236, 21.Google Scholar
Larson, R. B.: 1972b, Monthly Notices Roy. Astron. Soc. 156, 437.CrossRefGoogle Scholar
Larson, R. B.: 1974a, Monthly Notices Roy. Astron. Soc. 166, 585.Google Scholar
Larson, R. B.: 1974b, Monthly Notices Roy. Astron. Soc. 169, 229.CrossRefGoogle Scholar
Larson, R. B. and Tinsley, B. M.: 1974, Astrophys. J. 192, 293.Google Scholar
Lecar, M. and Cohen, L.: 1972, in Lecar, M. (ed.), Gravitational N-Body Problem, D. Reidel Publ. Co., Dordrecht-Holland, p. 262.Google Scholar
Liller, M. H.: 1960, Astrophys. J. 132, 306.Google Scholar
Liller, M. H.: 1966, Astrophys. J. 146, 28.Google Scholar
Lynden-Bell, D.: 1967, Monthly Notices Roy. Astron. Soc. 136, 101.Google Scholar
McClure, R. D.: 1969, Astron. J. 74, 50.Google Scholar
Miller, R. H. and Prendergast, K. H.: 1962, Astrophys. J. 136, 713.CrossRefGoogle Scholar
Oort, J. H.: 1970, Astron. Astrophys. 7, 381.Google Scholar
Oort, J. H.: 1974, in Shakeshaft, J. R. (ed.), ‘The Formation and Dynamics of Galaxies’, IAU Symp. 58, 375.Google Scholar
Ostriker, J. P., and Peebles, P. J. E.: 1973, Astrophys. J. 186, 467.Google Scholar
Ostriker, J. P., and Thuan, T. X.: 1975, Astrophys. J. (in press).Google Scholar
Peebles, P. J. E.: 1971, Astron. Astrophys. 11, 377.Google Scholar
Peebles, P. J. E.: 1972, Comments Astrophys. Space Phys. 4, 53.Google Scholar
Peebles, P. J. E.: 1974a, Astrophys. J. Letters 189, L51.Google Scholar
Peebles, P. J. E.: 1974b, in Shakeshaft, J. R. (ed.), ‘The Formation and Dynamics of Galaxies’, IAU Symp. 58, 55.Google Scholar
Peebles, P. J. E. and Dicke, R. H.: 1968, Astrophys. J. 154, 891.Google Scholar
Roberts, M. S. and Rots, A. H.: 1973, Astron. Astrophys. 26, 483.Google Scholar
Sandage, A. R.: 1972, Astrophys. J. 176, 21.CrossRefGoogle Scholar
Saslaw, W. C.: 1971, Monthly Notices Roy. Astron. Soc. 152, 341.Google Scholar
Saslaw, W. C.: 1972, Astrophys. J. 177, 17.Google Scholar
Shields, G. A.: 1974, Astrophys. J. 193, 335.Google Scholar
Silk, J. I. and Lea, S. M.: 1973, Astrophys. J. 180, 669.Google Scholar
Spinrad, H., Gunn, J. E., Taylor, B. J., McClure, R. D., and Young, J. W.: 1971, Astrophys. J. 164, 11.CrossRefGoogle Scholar
Spinrad, H., Smith, H. E., and Taylor, B. J.: 1972, Astrophys. J. 175, 649.Google Scholar
Spitzer, L.: 1971, in O'Connell, D. J. K. (ed.), Nuclei of Galaxies, American Elsevier, New-York, p. 443.Google Scholar
Toomre, A. and Toomre, J.: 1972, Astrophys. J. 178, 623.Google Scholar
Tremaine, S. D., Ostriker, J. P., and Spitzer, L.: 1975, Astrophys. J. 196, 407.Google Scholar
Van Houten, C. J.: 1971, Bull. Astron. Inst. Neth. 16, 1.Google Scholar
Wilson, C. P.: 1975, Astron. J. 80, 175.Google Scholar