PULSAR RADIO-EMISSION

被引：0
|
作者：
KUNDT, W
机构：
[1] Institut für Astrophysik der Universität Bonn, Bonn, D-53121
来源：
SPACE SCIENCE REVIEWS | 1994年 / 68卷 / 1-4期
关键词：
PULSARS; GENERAL; MAGNETOSPHERE; PULSAR WIND; MASERS; COHERENT RADIOEMISSION;
D O I：
10.1007/BF00749164
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
25 years after their discovery, pulsars still pose fundamental problems, in particular when the whole range of their periods P is considered: 1.56 ms less-than-or-equal-to P less-than-or-equal-to 5.09 s. This communication reviews my understanding of the pulsar magnetosphere, windzone, and (coherent) radio emission. New are details of the preferred magnetic structure, wind generation, and amplification of the emitted (pseudo) curvature radiation, the inferred brightness of which exceeds that of all other terrestrial and astrophysical sources by many orders of magnitude.
引用
收藏
页码：357 / 362
页数：6
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