High energy cosmic ray spectroscopy. III. Further analyses

被引:39
作者
Erlykin, AD
Wolfendale, AW
机构
[1] Univ Durham, Dept Phys, Durham DH1 3LE, England
[2] PN Lebedev Phys Inst, Moscow 117924, Russia
关键词
D O I
10.1016/S0927-6505(97)00053-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In recent papers (A.D. Erlykin and A.W. Wolfendale, Astropart. Phys. 7 (1997) 1, 203) we presented evidence favouring the identification of "structure" in the size spectrum of cosmic ray electrons and muons with heavy nuclei originating in a single local, recent, supernova. Inevitably, such a claim, in a field that is notoriously difficult, has not met with universal agreement. In the present work we add more recent evidence and address the criticisms. Almost all of the evidence considered appears to support our claim; the remainder is neutral. (C) 1998 Elsevier Science B.V.
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页码:265 / 281
页数:17
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