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The X-ray Appearance of Supernova Remnants in Tenuous Media
Published online by Cambridge University Press: 03 August 2017
Abstract
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By estimating the X-ray intensities of old supernova remnants in the disk-halo interface, deductions can be made about the ability of isolated supernovae to have created a coronal halo.
- Type
- III. Theory and Modelling
- Information
- Copyright
- Copyright © Kluwer 1991
References
REFERENCES
Cioffi, D. F. (1990) in
Physical Processes in Hot Cosmic Plasmas
, eds. Brinkmann, W., Fabian, A. C., Giovannelli, F., Kluwer, Dordrecht, p. 1
Google Scholar
Cioffi, D. F., McKee, C. F. (1988) in
Proc of IAU Coll. 101, Supernova Remnants and the Interstellar Medium
, eds. Roger, R. S., Landecker, T. L., C.U.P., Cambridge, p. 435
Google Scholar
Sedov, L. I. (1959)
Similarity & Dimensional Methods in Mechanics
, Academic Press, NY
Taylor, G. I.
(1950) Proc. Roy. Soc. London 201A, 159
Google Scholar
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