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arXiv 0903.2606astro-ph.CO
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Blazar AO 0235+164和1ES 2321+419的长时相X射线光变曲线的近周期起伏

Nearly Periodic Fluctuations in the Long Term X-ray Light Curves of the Blazars AO 0235+164 and 1ES 2321+419

Bindu Rani, Paul J. Wiita, Alok C. Gupta

摘要:

我们已经进行了结构功能分析的罗西X射线定时探测器全天监测数据搜索的变化,在24个耀变体使用的数据列车,每个超过12年。尽管其中20个观测到了名义周期,但绝大多数观测到的“周期”都与仪器观测到的年变化有关,尽管如此,对耀变体AO 0235+164观测到了一个约为17天的明显的实际周期分量,离散关联函数和周期图分析证实了这一点。对于1ES 2321+419,通过所有这些方法检测到具有约420天的近周期性的可变性成分。我们讨论了几种可能的解释,这些近周期性的组件,并得出结论,他们最有可能产生的交叉点的冲击波传播的相对论性喷流,具有螺旋结构。

英文摘要:

We have performed a structure function analysis of the Rossi X-ray Timing Explorer All Sky Monitor data to search for variability in 24 blazars using data trains that each exceed 12 years. Although 20 of them show nominal periods though this technique, the great majority of these `periods' are clearly related to yearly variations arising from the instrument.Nonetheless, an apparently real periodic component of about 17 days was detected for the blazar AO 0235+164 and it was confirmed by discrete correlation function and periodogram analyses. For 1ES 2321+419 a component of variability with a near periodicity of about 420 days was detected by all of these methods. We discuss several possible explanations for these nearly periodic components and conclude that they most likely arise from the intersections of a shock propagating down a relativistic jet that possesses a helical structure.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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