Magnetic Fields of Radio Pulsars

被引：13
|
作者：
Nikitina, E. B. [1 ]
Malov, I. F. [1 ]
机构：
[1] Russian Acad Sci, Lebedev Phys Inst, Pushchino Radio Astron Observ, Pushchino 142290, Moscow Oblast, Russia
来源：
ASTRONOMY REPORTS | 2017年 / 61卷 / 07期
基金：
俄罗斯基础研究基金会;
关键词：
MAGNETOSPHERES; INTERPULSES; MECHANISM; EMISSION; AXIS;
D O I：
10.1134/S1063772917070058
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The mechanism of magnetodipole braking of radio pulsars is used to calculate new values of the surface magnetic fields of neutron stars. The angles beta between the spin axes and magnetic moments of the neutron stars were estimated for 376 radio pulsars using three different methods. It is shown that small inclinations of magnetic axes dominate. The equatorial magnetic fields for the considered sample of pulsars are calculated using the beta values obtained. As a rule, these magnetic fields are a factor of a few higher than the corresponding values in known catalogs.
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页码：591 / 611
页数：21
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