No CrossRef data available.
Article contents
Observational Constraints on Cosmological Models
Published online by Cambridge University Press: 12 April 2016
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.
Cosmological models for structure formation are severely constrained by several of the recent observational results. We now have observations which probe the power spectrum of fluctuations from about 0.5 h−1 Mpc to 3000 h−1 Mpc. These probes and the constraints they imply on models for structure formation are reviewed.
- Type
- XII. Cosmology
- Information
- International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 470 - 477
- Copyright
- Copyright © Astronomical Society of the Pacific 1995
References
Bagla, J.S. & Padmanabhan, T., 1993, IUCAA preprint 22/93, in Proc. of VI IAU Asian Pacific Reg. Mtg, in pressGoogle Scholar
Bertschinger, E., Dekel, A., Faber, S.M., Dressler, A. & Berstein, D., ApJ, 1990, 364, 370
Google Scholar
Efstathiou, G., Kaiser, N., Saunders, W., Lawrence, A., Rowan-Robinson, M., Ellis, R.S. & Frenk, C.S., 1990, MNRAS, 247, 10p
Google Scholar
Schuster, J., Gaier, T., Gunderson, J., Meinhold, P., Koch, T., Seiffert, M., Wueusche, C.A. & Lubin, P., 1993
ApJ
412, L47
Google Scholar
You have
Access