Abstract
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.
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© 1983 IAU
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Stewart, G.C., Fabian, A.C., Seward, F.D. (1983). An X-Ray Halo around Cassiopeia A. In: Danziger, J., Gorenstein, P. (eds) Supernova Remnants and their X-Ray Emission. International Astronomical Union / Union Astronomique Internationale, vol 101. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7231-5_7
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DOI: https://doi.org/10.1007/978-94-009-7231-5_7
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-1667-5
Online ISBN: 978-94-009-7231-5
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