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The X-ray Appearance of Supernova Remnants in Tenuous Media
Published online by Cambridge University Press: 03 August 2017
Abstract
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.
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- III. Theory and Modelling
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- Copyright © Kluwer 1991