STRONGLY MAGNETIC WHITE-DWARF BINARIES IN GLOBULAR-CLUSTERS

被引：3

作者：

RAY, A ^{[1
]}

CHANMUGAM, G ^{[1
]}

机构：

[1] LOUISIANA STATE UNIV,DEPT PHYS & ASTRON,BATON ROUGE,LA 70803

来源：

ASTROPHYSICAL JOURNAL | 1990年 / 350卷 / 01期

关键词：

Clusters: globular; Stars: binaries; Stars: magnetic; Stars: white dwarfs;

D O I：

10.1086/185655

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We predict that globular clusters are likely to contain a new class of magnetic cataclysmic variables (CVs) with significantly high fields (50≤B≤500 MG) which is unknown among the CVs in the solar neighborhood. In addition, we make estimates of their expected X-ray luminosities and propose that X-ray surveys combined with optical/UV observations should lead to the detection of the brightest of them. Specific target globular clusters with high probability of detection of these sources are given.

引用

页码：L9 / L12

页数：4

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