A possible mechanism for flattening of pulsar spectra at high frequencies

被引：0
|
作者：
Malov, IF [1 ]
机构：
[1] PN Lebedev Phys Inst, Pushchino Radio Astron Observ, Pushchino 142292, Russia
来源：
PULSAR ASTRONOMY - 2000 AND BEYOND: IAU COLLOQUIUM 177 | 2000年 / 202卷
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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页码：395 / 396
页数：2
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