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5. The emission positions of kHz QPOs and Kerr spacetime influence

The emission positions of kHz QPOs and Kerr spacetime influence

来源 :中国科学：物理学、力学、天文学英文版 | 被引量 : 0次 | 上传用户：binhuchen007

【摘 要】

：

Based the Alfven wave oscillation model(AWOM) and relativistic precession model(RPM) for twin kHz QPOs,we estimate the emission positions of most detected kHz Q

【出 处】

：

中国科学：物理学、力学、天文学英文版

【发表日期】

：

2010年S1期

【关键词】

：

KHZ QPO neutron star LOW-MASS X-ray BINARIES kHz QPOneutron starlow-mass X-ray b 

【基金项目】

：

supported by the National Basic Research Program of China (Grant No. 2009CB824800),the National Natural Science Foundation of China (Grant No. 10773017)

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Based the Alfven wave oscillation model(AWOM) and relativistic precession model(RPM) for twin kHz QPOs,we estimate the emission positions of most detected kHz QPOs to be at r=18+/-3 km(R/15 km),except Cir X-1 at r-30+/-5 km(R/15 km).For the proposed Keple

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