Strange stars in Low-Mass Binary Pulsar systems

被引：2
作者：
Horvath, JE
机构：
[1] Univ Sao Paulo, Inst Astron & Geofis, BR-04301904 Sao Paulo, Brazil
[2] Univ Arizona, Steward Observ, Tucson, AZ USA
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 1999年 / 8卷 / 06期
关键词：
D O I：
10.1142/S021827189900047X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Based on observational facts and a variety of theoretical arguments we discuss in this work the possibility that pulsars in Low-Mass Binary Pulsar systems could be strange stars rather than neutron stars. It is shown that, although subject to reasonable uncertainties, the consideration of the physics of the SQM core and thin normal crusts leads to the prediction of several observed features of the magnetic field history of these systems within this working hypothesis.
引用
收藏
页码：669 / 675
页数：7
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