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The X-ray Appearance of Supernova Remnants in Tenuous Media

Published online by Cambridge University Press:  03 August 2017

Denis F. Cioffi
Denis F. Cioffi*
Affiliation:
Physics Department North Carolina State University Raleigh, NC 27695-8202 USA

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
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 355 - 358
Copyright
Copyright © Kluwer 1991 

References

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