Hard X-Rays from the Crab Pulsar

Details Hard X-Rays from the Crab Pulsar Hard X-Rays from the Crab Pulsar

Oct 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224...50f&link_type=abstract

Nature, Volume 224, Issue 5214, pp. 50-51 (1969).

Physics

23

Scientific paper

WE have recently measured the pulsed emission of high energy X-rays from the Crab Nebula pulsar NP 0532. Pulsation of the low energy X-ray flux with the characteristic period and double peaks seen in the radio1 and optical2 spectral regions was first reported by Fritz et al.3 and later by Bradt et al.4. The latter were able to establish correspondence between the visible and X-ray pulses by simultaneous observations. Fishman et al.5 have reported that the pulsar also appears in data taken in 1967 at the high end (greater than 35 keV) of the Crab X-ray spectrum.

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