New results on transient neutron-star low-mass X-ray binaries in quiescence

被引：11
|
作者：
Campana, S [1 ]
Stella, L
机构：
[1] INAF, Osservatorio Astron Brera, I-23807 Merate, LC, Italy
[2] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Roma, Italy
来源：
NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2004年 / 132卷
关键词：
D O I：
10.1016/j.nuclphysbps.2004.04.077
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
We review the main observational properties of neutron star low mass transients in quiescence. We first survey the discoveries of BeppoSAX. We then focus on recent discoveries by Chandra and XMM-Newton, with special emphasis on the detection of the quiescent counterpart of SAX J1808.4-3658 and the study of variability in the quiescent state.
引用
收藏
页码：427 / 434
页数：8
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