Weakly radiating radio pulsars

被引：7

作者：

Beskin, VS

Nokhrina, EE

机构：

[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 119991, Russia

[2] Moscow Phys Tech Inst, Dolgoprudnyi 141700, Moscow Oblast, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2004年 / 30卷 / 10期

基金：

俄罗斯基础研究基金会;

关键词：

pulsars; eutron stars; and black holes; radio pulsars;

D O I：

10.1134/1.1808055

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyze the statistical distribution of weakly radiating pulsars, i.e., radio pulsars that have passed to the stage of an orthogonal rotator during the evolution of the inclination angle X. We discuss in detail the factors that lead to a significant reduction in the energy losses for this class of objects. We have determined the number of weakly radiating radio pulsars and their distribution in spin period P. The predictions of a theory based on the model of current losses are shown to be consistent with observational data. (C) 2004 MAIK "Nauka/Interperiodica".

引用

页码：685 / 693

页数：9

共 9 条

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Mestel L., 1999, STELLAR MAGNETISM

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[9]

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