Pulsar reflections within the Crab Nebula
β Scribed by A. G. Lyne; R. S. Pritchard; F. Graham-Smith
- Publisher
- John Wiley and Sons
- Year
- 2001
- Tongue
- English
- Weight
- 118 KB
- Volume
- 321
- Category
- Article
- ISSN
- 0035-8711
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π SIMILAR VOLUMES
The Crab Pulsar is a relatively young neutron star. The Pulsar is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was observed on Earth in the year 1054. The Crab Pulsar has been extensively observed in the gamma-ray energy band by the Large Area Telescope (LAT), the m
We present the results of a CCD monitoring campaign of the continuum emission from the central region of the Crab nebula, amounting to 17 epochs spread over 3.5 years. The data provide clear evidence that the brightest wisps move outward from the pulsar at mildly relativistic velocities. This motion