Peculiar differences in radio and X-ray synchrotron radiation from pulsar wind nebulae

被引：0

作者：

Dickel, JR ^{[1
]}

Wang, SY ^{[1
]}

机构：

[1] Univ Illinois, Dept Astron, Urbana, IL 61801 USA

来源：

YOUNG NEUTRON STARS AND THEIR ENVIRONMENTS | 2004年 / 218期

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D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Several Crab-type supernova remnants appear to have very bright non-thermal X-ray cores just around the pulsar or expected pulsar. This X-ray brightness is often not matched by a corresponding increase in radio emission. The best example of this phenomenon is in N157B in the LMC. G21.5-0.9 and possibly 3C 58 also show it while the Crab Nebula and 0540-69.3 do not. Some method to enhance the higher energy particles must be present in these objects.

引用

页码：221 / 224

页数：4

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