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An X-ray Halo Around Cassiopeia A
Published online by Cambridge University Press: 04 August 2017
Abstract
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We report on evidence for weak large scale (r ≥ 6 arcmin) X-ray emission from Cassiopeia A. We investigate several mechanisms for producing such an X-ray halo. Further observations will be required to determine which mechanism is operative.
- Type
- I. Young Supernova Remnants
- Information
- Copyright
- Copyright © Reidel 1983
References
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