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
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D O I：
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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.
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页码：47 / 48
页数：2
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