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Fine-Scale Anisotropy of the Cosmic Microwave Background Radiation

Published online by Cambridge University Press:  07 February 2017

Paul E. Boynton*
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, Wash., U.S.A.

Extract

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In keeping with the title of Symposium No. 63, I would like to confront the assembly with a short review of observational upper limits on the amplitude of intensity fluctuations in the microwave background radiation on angular scales of less than one degree. These fluctuations are presently of interest for at least two important cosmological concerns:

Type
Part III: Relic Radiation
Copyright
Copyright © Reidel 1974 

References

Boynton, P. E. and Partridge, R. B.: 1973, Astrophys. J. 181, 243.Google Scholar
Carpenter, R. L., Gulkis, S., and Sato, T.: 1973, Astrophys. J. Letters 182, L61.Google Scholar
Conklin, E. K. and Bracewell, R. N.: 1967, Nature 216, 777.CrossRefGoogle Scholar
Hazard, C. and Salpeter, E. E.: 1969, Astrophys. J. Letters 157, L87.Google Scholar
Kiang, T.: 1961, Monthly Notices Roy. Astron. Soc. 122, 263.Google Scholar
Parijskij, Yu. N.: 1973, Astrophys. J. Letters 180, L47.Google Scholar
Parijskij, Yu. N. and Pyatunina, T. B.: 1970, Astron. Zh. 47, 1337.Google Scholar
Penzias, A. A., Schraml, J., and Wilson, R. W.: 1969, Astrophys. J. Letters 157, L49.Google Scholar
Smith, M. G. and Partridge, R. B.: 1970, Astrophys. J. 159, 737.Google Scholar