Burst-only sources: probing type I X-ray bursters at low persistent luminosities

被引：21

作者：

Cornelisse, R ^{[1
]}

in 't Zand, JJM

Kuulkers, E

Heise, J

Verbunt, F

Cocchi, M

Bazzano, A

Natalucci, L

Ubertini, P

机构：

[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England

[2] SRON, Natl Inst Space Res, NL-3584 CA Utrecht, Netherlands

[3] Univ Utrecht, Inst Astron, NL-3508 TA Utrecht, Netherlands

[4] ESA, Estec, Sci Operat & Data Syst Devis, SCi,SDG, NL-2201 AZ Noordwijk, Netherlands

[5] Area Ric Roma Tor Vergata, Ist Astrofis Spaziale, I-00133 Rome, Italy

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2004年 / 132卷

关键词：

D O I：

10.1016/j.nuclphysbps.2004.04.087

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：

The Wide Field Cameras onboard BeppoSAX observed 9 type I X-ray bursters without detectable persistent emission around the burst. According to the standard theory of X-ray bursts these sources should be in the lowest mass-accretion regime, opening the possibility to study this regime for the first time. We compare the sources with the burst theory, and show that the evidence of a new sub-class of low mass X-ray binaries, the burst-only source, is still meagre.

引用

页码：518 / 523

页数：6

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