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LONG-TERM VARIATIONS IN THE PULSE EMISSION FROM PSR J0737-3039B

机译:PSR J0737-3039B的脉冲发射的长期变化

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摘要

Analysis of 20 months of observations at the Parkes radio telescope shows secular changes in the pulsed emission from J0737—3039B, the 2.77 s pulsar of the double-pulsar system. Pulse profiles are becoming single-peaked in both bright phases of the orbital modulation, although there is no clear variation in overall pulse width. The shape of the orbital modulation is also varying systematically, with both bright phases shrinking in longitude by ~7° yr~(-1). However, the combined span of the two bright phases is relatively constant, and together they are shifting to higher longitudes at a rate of ~3° yr~(-1). We discuss the possible contributions of geodetic precession and periastron advance to the observed variations.
机译:对Parkes射电望远镜进行的20个月观察的分析显示,J0737-3039B(双脉冲系统的2.77 s脉冲星)的脉冲发射出现了长期变化。尽管总体脉冲宽度没有明显变化,但在轨道调制的两个明亮阶段,脉冲轮廓都变得单峰。轨道调制的形状也有系统地变化,两个亮相的经度都缩小了〜7°yr〜(-1)。然而,两个亮相的组合跨度是相对恒定的,它们一起以〜3°yr〜(-1)的速率向较高的经度移动。我们讨论了大地岁差和近地星前移对观测到的变化的可能贡献。

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