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Final Remarks: Connections between Chemical and Dynamical Evolution

Published online by Cambridge University Press:  12 April 2016

Beatrice M. Tinsley
Beatrice M. Tinsley*
Affiliation:
Yale University Observatory

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Dynamical processes strongly affect the chemical enrichment of gas in galaxies, so abundances in stars and the Interstellar medium can be used as probes of the dynamical history of the Galaxy. By way of tying together some diverse points, rather than summarizing the conference, I shall discuss some examples of connections between chemical and dynamical evolution. The first section of this paper mentions some of the well-known ways in which dynamical processes can affect chemical evolution, in order to outline a theoretical background to the use of abundances as clues to dynamics.

Information

Type
Part V: Final Remarks
Information
International Astronomical Union Colloquium , Volume 45: Chemical and Dynamical Evolution of our Galaxy , September 1977, pp. 309 - 319
Copyright
Copyright © Geneva Observatory 1977

References

Audouze, J., and Tinsley, B.M..: 1976, Ann. Rev. Astron. Astrophys., 14, 43 (AT).Google Scholar
Biermann, P. and Biermann, L.: 1977, Astron. Astrophys., 55, 63.Google Scholar
Burki, G.: 1977, Astron. Astrophys., 57, 135.Google Scholar
Conti, P. S., and Burnichan, M.-L.: Astron. Astrophys., 38, 467.Google Scholar
Conti, P. S., Greenstein, J. L., Spinrad, H., Wallerstein, G., and Vardya, M.S..: 1967, Astrophys. J., 148, 105.CrossRefGoogle Scholar
Cowley, A. P., Hartwick, F. D. A., and Sargent, W. L. W.: 1977, preprint.Google Scholar
Cox, D. P. and Smith, B.W..: 1976, Astrophys. J., 203, 361.Google Scholar
Cruz-Gonzalez, C., Recillas-Cruz, E., Costero, R., Peimbert, M., and Torres-Peimbert, S.: 1974, Revista Mexicana de Astronomia y Astrofisica, 1, 211.Google Scholar
Dearborn, D., Tinsley, B. M., and Schramm, D. N. 1978, preprint.Google Scholar
Demarque, P. and McClure, R.D..: 1977, in Tinsley, B. M. and Larson, R. B. (eds.), ‘The Evolution of Galaxies and Stellar Populations.’ Yale University Observatory, New Haven, p. 199.Google Scholar
Eggen, O. J., Lynden-Bell, D., and Sandage, A.: 1962, Astrophys. J. 136, 748.Google Scholar
Freeman, K.C..: 1977, in Tinsley, B. M. and Larson, R. B. (eds.), ‘The Evolution of Galaxies and Stellar Populations,’ Yale University Observatory, New Haven, p. 133.Google Scholar
Hartwick, F. D. A.: 1976, Astrophys. J., 209, 418.Google Scholar
Kirshner, R. P. and Oke, J.B..: 1975, Astrophys. J., 200, 574.CrossRefGoogle Scholar
Lambert, D. L., Sneden, C., and Ries, L.M..: 1974, Astrophys. J., 188, 97.Google Scholar
Larson, R.B..: 1972, Nature Phys. Sci., 236, 7.CrossRefGoogle Scholar
Ostriker, J. P., Richston, D. O., and Thuan, T.X..: 1974, Astrophys. J. (Letters), 188, L87.CrossRefGoogle Scholar
Ostriker, J. P. and Thuan, T.X..: 1975, Astrophys. J., 202, 353.Google Scholar
Pagel, B. E. J. and Patchett, B.E..: 1975, Monthly Notices Roy. Astron. Soc, 172, 13.Google Scholar
Reeves, H.: 1972, Astron. Astrophys., 19, 215.Google Scholar
Sargent, W. L. W.: 1977, in Tinsley, B. M. and Larson, R. B. (eds.), ‘The Evolution of Galaxies and Stellar Populations.’, Yale University Observatory, New Haven, p. 427.Google Scholar
Schmidt, M.: 1963, Astrophys. J., 137, 758.Google Scholar
Schmidt, M.: 1975, Astrophys. J., 202, 22.Google Scholar
Searle, L.: 1972, in Delplace, M. and Cayrel de Strobel, G. (eds.), ‘Stellar Ages’, I.A.U. Colloquium No. 17, Meudon Observatory, Paris.Google Scholar
Searle, L.: 1977, in Tinsley, B. M. and Larson, R. B. (eds.), ‘The Evolution of Galaxies and Stellar Populations,’ Yale University Observatory, New Haven p. 219.Google Scholar
Shields, G. A. and Tinsley, B.M..: 1974, Astrophys. J., 193, 335.CrossRefGoogle Scholar
Stothers, R. and Chin, C.: 1977, Astrophys. J., 211, 189.Google Scholar
Strom, S. E., Strom, K. M., and Grasdalen, G.L..: 1975, Ann. Rev. Astron. Astrophys., 13, 187.Google Scholar
Talbot, R.J..: 1974, Astrophys. J., 189, 209.Google Scholar
Talbot, R. J. and Arnett, W.D..: 1973, Astrophys. J., 186, 69.Google Scholar
Talbot, R. J. and Arnett, W.D..: 1975, Astrophys. J., 197, 551.CrossRefGoogle Scholar
Tammann, G.A..: 1977, in Schramm, D. N. (ed.), ‘Supernovae,’ D. Reidel Pub. Co., Dordrecht, p. 95.Google Scholar
Tinsley, B.M..: 1975, Astrophys. J., 197, 159.Google Scholar
Tinsley, B.M..: 1977a, in Schramm, D. N. (ed.), ‘Supernovae,’ D. Reidel Pub. Co., Dordrecht, p. 117.Google Scholar
Tinsley, B.M..: 1977b, Astrophys. J., 216, 548.CrossRefGoogle Scholar
Truran, J. W. : 1973, Commments Astrophys. Space Phys., 5, 117.Google Scholar
van den Bergh, S.: 1962, Astron. J., 67, 486.Google Scholar