A possible mechanism for flattening of pulsar spectra at high frequencies

被引：0

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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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中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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页码：395 / 396

页数：2

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