Arrival-time analysis for a pulsar in a binary system.
Arrival-time analysis for a pulsar in a binary system.
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DOI：
10.1086/154315
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发表时间：
1976-04
期刊：
影响因子：
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通讯作者：
R. Blandford;S. Teukolsky
中科院分区：
文献类型：
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作者：
R. Blandford;S. Teukolsky
本文描述了一种从脉冲双星PSR 1913+16的轨道根数及其可能的长期变化分析脉冲到达时间的方法。估计给出必要的时间来测量这种长期的变化，并检测各种相对论效应。如果测量误差约。1毫秒是主要的误差来源和约。1000独立的意见，每年进行，然后约。5年的观测是必要的组件质量的动态测定准确到10%和约。15年的引力辐射的可能检测。其他来源的错误进行了简要讨论。（AIP）
A method is described for analyzing the arrival times of pulses from the binary pulsar PSR 1913+16, in terms of the orbital elements and their possible secular variations. Estimates are given for the times necessary to measure such secular changes and to detect various relativistic effects. If measurements errors approx.1 ms are the dominant source of error and approx.1000 independent observations are made per year, then approx.5 years of observations are necessary for a dynamical determination of the component masses accurate to 10 percent and approx.15 years for the possible detection of gravitational radiation. Other sources of error are briefly discussed. (AIP)