Advertisement

Panel Contribution—IAU Symposium 168

  • R. B. Partridge
Part of the International Astronomical Union/Union Astronomique Internationale book series (IAUS, volume 168)

Abstract

These brief comments will reflect the point of view of an observer, rather than a theorist. They will also be quite informal, as were the remarks I made while at the symposium in The Hague. Finally, I will restrict myself to relatively low energy proton backgrounds-roughly speaking from 105–101eV. I fear that will slight the important work being done by our colleagues on the X-ray and gamma ray backgrounds, but those topics were nicely covered in the symposium itself.

Keywords

Cosmic Microwave Background Radiation Interplanetary Dust Galaxy Evolution Cosmological Background Large Angular Scale 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Eggen, O. J., Lynden-Bell, D., and Sandage, A. R. 1962, Ap. J., 136 748ADSCrossRefGoogle Scholar
  2. Gush, H. P., Halpern, M., and Wishnow, E. H. 1990, Phys. Rev. Lett. 65, 537Google Scholar
  3. Mather, J. C., et. al. 1990, Ap. J. (Letters), 354, L37ADSCrossRefGoogle Scholar
  4. Mather, J.C., et. al. 1994, Ap.J., 420, 439ADSCrossRefGoogle Scholar
  5. Partridge, R. B., and Peebles, P. J. E., 1967, Ap. J., 147, 868ADSCrossRefGoogle Scholar
  6. Smoot, G.F., et. al. 1992, Ap.J.(Letters), 396, L1Google Scholar

Copyright information

© International Astronomical Union 1996

Authors and Affiliations

  • R. B. Partridge
    • 1
  1. 1.Haverford CollegeUSA

Personalised recommendations