Other
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.233..305s&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 233, July 15, 1988, p. 305-319.
Other
53
Crab Nebula, Emission Spectra, Optical Polarization, Pulsars, Background Radiation, Polarization Characteristics, Radio Emission, Relativistic Particles
Scientific paper
The optical polarizations of the Crab Nebula Pulsar has been remeasured, using a new determination of the polarization of the background emission from the nebula. The emission from the pulsar at minimum light is 47 + or - 10 percent polarized at position angle 130 deg. The polarization characteristics of the two pulse components are remarkably similar. The observations support a model in which optical and other high-energy radiation is emitted from close to the light cylinder, the two pulses corresponding to the two magnetic poles in a nearly orthogonal rotator.
Dick S. B. J.
Graham Smith F.
Jones H. P. D.
Pike David C.
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