The shadow of a pulsar and the inward radio emission in pulsar magnetosphere

被引：3
|
作者：
Dyks, J. [1 ]
Frackowiak, M.
Slowikowska, A.
Rudak, B.
Bing Zhang
机构：
[1] Ctr Astron M Kopernika PAN, Torun, Poland
[2] Univ Nevada, Dept Phys, Las Vegas, NV 89154 USA
[3] CA UMK, Torun, Poland
来源：
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2006年 / 6卷
关键词：
pulsars : general; pulsars; individual; (B0950+08; B1822-09; B1929+10; J0437-4715);
D O I：
10.1088/1009-9271/6/S2/18
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We discuss observational facts that can be interpreted in terms of inward emission in pulsar magnetosphere. These include the main-pulse/interpulse anticorrelation in B1822-09 and the locations of emission and absorption features in the pulse profile of B0950+08. Weaknesses of geometrical models employing the inward emission are carefully discussed.
引用
收藏
页码：85 / 89
页数：5
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