Denis F. Cioffi
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.
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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.
Key concepts: Supernova, Halo, Astrophysics, Physics, Coronal plane, Astronomy, Near-Earth supernova, Galaxy