Published August 1987 | Version v1
Journal article

Scanning modulation collimator observation of the high-energy X-ray source in the Crab Nebula

  • 1. Tokyo Univ., Japan
  • 2. California Univ., La Jolla

Description

Two-dimensional maps of the 22-64 keV emission from the Crab Nebula with an angular resolution of 15 arcsec has been synthesized. The maps are generated by application of a maximum entropy method operating on a series of one-dimensional scans obtained with a balloon-borne modulation collimator telescope. The two-dimensional size, shape and orientation of the hard X-ray nebula relative to the pulsar have been measured for the first time. The implications of these results for models of electron transport in the Crab are discussed, and the geometry of the observed X-ray nebula is related to other features of the Crab Nebula system. 63 references

Additional details

Publishing Information

Journal Title
Astrophys. J.
Journal Volume
319
Series
Astrophys. J.
Journal Page Range
416-425
ISSN
0004-637X
CODEN
ASJOA