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Individual Radio Pulses from NP 0531

Published online by Cambridge University Press:  07 February 2017

J. M. Sutton ,
D. H. Staelin  and
R. M. Price
J. M. Sutton
Affiliation:
NRAO, Green Bank, W. Va. U.S.A.∗ IOTA, University of Cambridge, U.K.
D. H. Staelin
Affiliation:
Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.
R. M. Price
Affiliation:
Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.

Abstract

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Observations with a swept frequency machine show that the shapes of individual pulses from NP 0531 are truncated exponentials with widths proportional to λ~4, consistent with the broadening arising from scattering in the interstellar medium. A histogram of pulse intensity reveals two different populations. The very strong pulses are associated only with the main pulse and interpulse.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 97 - 102
Copyright
Copyright © Reidel 1971 

References

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