High field magnetic white dwarfs, pulsars, magnetars, and their main sequence progenitors

被引：0
|
作者：
Ferrario, Lilia [1 ]
Wickramasinghe, D. T. [1 ]
机构：
[1] Australian Natl Univ, Canberra, ACT 0200, Australia
来源：
15TH EUROPEAN WORKSHOP ON WHITE DWARFS, PROCEEDINGS | 2007年 / 372卷
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：
Super-strong magnetic fields are observed in both white dwarfs and neutron stars. In this paper, we present calculations that highlight the commonality of their properties and the implications for their main sequence progenitors.
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页码：163 / +
页数：2
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