Abstract
It is shown that if the recently discovered hypernova events are intrinsically energetic spherically symmetric explosions of massive stars than they can leave after themselves very large diameter (up to 500 pc) nonthermal radio shells with spectral properties like ordinary shell type radio supernova remnants (SNRs). The properties of such shells are modeled and compared with the statistics of large diameter SNRs.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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