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Searches for Primeval Galaxies - Past, Present, and Future

Published online by Cambridge University Press:  14 August 2015

Marc Davis
Marc Davis*
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Abstract

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Most models of galactic evolution include a high luminosity epoch of bright star formation at a redshift 2 < Z < 100. Past searches have failed to detect galaxies in their “primeval” state, but recent advances in detector technology will soon enable much improved searches that will very seriously constrain the evolutionary models. Using the CCD detectors on the Space Telescope offers the opportunity for a thousandfold improvement over present search limits. We review here several models of primeval galaxies and comment on their observability in present and future experiments.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 92: Objects of High Redshift , 1980 , pp. 57 - 64
Copyright
Copyright © Reidel 1980 

References

Butcher, H., and Oemler, A.E. 1978, Ap. J. , 219, 18.CrossRefGoogle Scholar
Davis, M., and Wilkinson, D.T. 1974, Ap. J. , 192, 251.CrossRefGoogle Scholar
Dube, R., Wilkinson, D.T., and Wickes, W.C. 1977, Ap. J. Lett. , 215, L51 CrossRefGoogle Scholar
Eggen, O.J., Lynden-Bell, D., and Sandage, H.R. 1962, Ap. J. , 136, 748.CrossRefGoogle Scholar
Kaufman, M., and Thuan, T.X. 1977, Ap. J. , 215, 11.CrossRefGoogle Scholar
Koo, D., and Kron, R. 1979, private communication.Google Scholar
Larson, R.B. 1974, M.N.R.A.S. , 166, 585.CrossRefGoogle Scholar
Larson, R.B., in Dynamics of Stellar Systems , I.A.U. Symposium No. 69 (Ed. Hayli, A.) (D. Reidel, Dordrecht, 1975) p. 247.CrossRefGoogle Scholar
Larson, R.B. 1976, Comments Astrophys. , 6, 139.Google Scholar
Loh, E., and Wilkinson, D.T. 1979, private communication.Google Scholar
MacKay, C. 1979, private communication.Google Scholar
Meier, D.L. 1976a, Ap. J. , 207, 343.CrossRefGoogle Scholar
Meier, D.L. 1976b, Ap. J. Lett. , 203, L103.CrossRefGoogle Scholar
Partridge, R.B., 1974, Ap. J. , 192, 241.CrossRefGoogle Scholar
Partridge, R.B., and Peebles, P.J.E. 1967a, Ap. J. , 147, 868.CrossRefGoogle Scholar
Partridge, R.B., and Peebles, P.J.E. 1976b, Ap. J. , 148, 377.CrossRefGoogle Scholar
Peebles, P.J.E. 1971, Physical Cosmology .Google Scholar
Searle, L., and Sargent, W. L. W. 1972, Ap. J. , 173, 25.CrossRefGoogle Scholar
Sunyaev, R.A., Tinsley, B.M., and Meier, D.L. 1978, Comments Astrophys. , 7, 183.Google Scholar
Tinsley, B.M. 1972, Ap. J. , 178, 319.CrossRefGoogle Scholar
Tinsley, B.M. 1977, Ap. J. , 211, 621.CrossRefGoogle Scholar
Tinsley, B.M. 1978, Ap. J. , 220, 816.CrossRefGoogle Scholar
Tinsley, B.M., and Larson, R.B. 1978, Ap. J. , 221, 554.CrossRefGoogle Scholar