High-frequency quasi-periodic oscillations in accreting neutron-star systems

被引：0
作者：
Mendez, Mariano [1 ]
机构：
[1] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
来源：
HIGHLIGHTS OF ASTRONOMY, VOL 15 | 2010年 / 15卷
关键词：
stars: neutron; stars: oscillations; X-rays: binaries; X-RAY BINARIES; MILLISECOND PULSAR; SPIN FREQUENCY; DISCOVERY; BURSTS; COLORS;
D O I：
10.1017/S1743921310008483
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Kilohertz quasi-periodic oscillations (kHz QPOs) are the fastest (almost coherent) variability measured in accreting X-ray binaries with a neutron-star primary. Here I review the role of the neutron-star spin in driving the frequencies of the kHz QPOs.
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页码：116 / 120
页数：5
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