High-energy emission from binary pulsars

被引：0
|
作者：
Tavani, M [1 ]
机构：
[1] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
来源：
MANY FACES OF NEUTRON STARS | 1998年 / 515卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Pulsars provide ideal accelerators of ultra-relativistic particles. High-energy emission is expected as the pulsar wind interacts with any gaseous surroundings. This interaction can be particularly strong in binaries with companion stars producing a strong mass outflow from their surfaces. We discuss here the theory and high-energy observations of pulsar binaries with pulsar/outflow interaction.
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页码：245 / 257
页数：13
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