The microlensing probability of the pulsars located in globular clusters

被引：0
|
作者：
Larchenkova, T [1 ]
机构：
[1] PN Lebedev Phys Inst, Ctr Astro Space, Moscow 117810, 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 ;
摘要：
We have used the effect of Shapiro delay of the pulsar radiation in the gravitational lensing approximation. The microlensing probabilities for pulsars located in globular clusters 47 Tuc (NGC 104) and M15 (7078) in the case of rather large impact parameters was calculated.
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页码：89 / 90
页数：2
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