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Optical Observations of the Crab Pulsar, and Searches for other Optical Pulsars

Published online by Cambridge University Press:  07 February 2017

Jerome Kristian
Jerome Kristian*
Affiliation:
Hale Observatories, Carnegie Institution of Washington and California Institute of Technology

Abstract

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The optical properties of the Crab nebula pulsar are reviewed. The Crab nebula pulsar has a high degree of constancy at optical wavelengths. No time variations over short or long periods have been detected; the light curve is nearly the same in all colors. The intensity and color of the pulsar are V = 16.5, B − V = +0.5, U − B = −0.45 and V − R = −0.75. There is no precursor as found at radio wavelengths and the main pulse contains 65 per cent of the total energy. No lines have been detected.

Searches for other pulsars have been unsuccessful.

Type
Session 2
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 87 - 90
Copyright
Copyright © Reidel 1971 

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