On the bottom magnetic fields of millisecond pulsars

被引：0

作者：

Mang, CM ^{[1
]}

机构：

[1] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia

来源：

YOUNG NEUTRON STARS AND THEIR ENVIRONMENTS | 2004年 / 218期

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：

The magnetic field strengths of most millisecond pulsars (MSPs) are about 10(8-9) gauss. The accretion-induced magnetic field evolution scenario here concludes that field decay is related to the accreted mass, that the minimum or bottom field stops at about 10(8) gauss for Eddington-limited accretion, and scales with the accretion rate as M-1/2. The possibility of low field (similar to 10(7) gauss) MSPs has been proposed for future radio observations.

引用

页码：47 / 48

页数：2

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