Hostname: page-component-84b7d79bbc-7nlkj Total loading time: 0 Render date: 2024-07-31T05:02:39.465Z Has data issue: false hasContentIssue false
  • English
  • Français

Galaxy Formation and Large-Scale Structures in a Two-Component Dark Matter Scenario

Published online by Cambridge University Press:  03 August 2017

Masayuki Umemura
Masayuki Umemura*
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan

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.

A universe dominated by both hot (HDM) and cold dark matter (CDM) is proposed. In this context, the new features for the formation of dwarf galaxies, Lyα clouds, galaxies, and large-scale structures are presented.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 427 - 428
Copyright
Copyright © Reidel 1988 

References

Brosch, N., and Gondhalekar, P. M. 1984, Astr. Ap. Letters, 140, 43.Google Scholar
Giovenelli, R. 1987, this volume.Google Scholar
Ikeuchi, S., and Norman, C. A. 1987, Ap. J., 312, 485.CrossRefGoogle Scholar
Kirshner, R. P., Oemler, A. Jr., Schechter, P. L., and Shectman, S. A. 1987, Ap. J., 314, 493.CrossRefGoogle Scholar
Peacock, J. A., Lumsden, S. L., and Heavens, A. F. 1987, M.N.R.A.S., in press.Google Scholar
Umemura, M., and Ikeuchi, S. 1985, Ap. J., 299, 583.CrossRefGoogle Scholar
White, S. D. M., Frenk, C. S., Davis, M., and Efstathiou, G. 1987, Ap. J., 313, 505.Google Scholar