首页> 外文期刊>The Astrophysical Journal. Letters >MULTIWAVELENGTH EVIDENCE FOR QUASI-PERIODIC MODULATION IN THE GAMMA-RAY BLAZAR PG 1553+113
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MULTIWAVELENGTH EVIDENCE FOR QUASI-PERIODIC MODULATION IN THE GAMMA-RAY BLAZAR PG 1553+113

机译:GAMMA-RAY BLAZAR PG 1553 + 113中准周期调制的多波长证据

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摘要

We report for the first time a gamma-ray and multiwavelength nearly periodic oscillation in an active galactic nucleus. Using the Fermi Large Area Telescope we have discovered an apparent quasi-periodicity in the gamma-ray flux (E > 100 MeV) from the GeV/TeV BL Lac object PG 1553+113. The marginal significance of the 2.18 +/- 0.08 year period gamma-ray cycle is strengthened by correlated oscillations observed in radio and optical fluxes, through data collected in the Owens Valley Radio Observatory, Tuorla, Katzman Automatic Imaging Telescope, and Catalina Sky Survey monitoring programs and Swift-UVOT. The optical cycle appearing in similar to 10 years of data has a similar period, while the 15 GHz oscillation is less regular than seen in the other bands. Further long-term multiwavelength monitoring of this blazar may discriminate among the possible explanations for this quasi-periodicity.
机译:我们首次报道了活跃的银河核中的伽马射线和多波长近乎周期性的振荡。使用费米大面积望远镜,我们发现了来自GeV / TeV BL Lac物体PG 1553 + 113的伽马射线通量(E> 100 MeV)中存在明显的准周期。通过在Owens谷射电天文台,Tuorla,Katzman自动成像望远镜和Catalina天空测量监视网收集的数据,通过在无线电和光通量中观察到的相关振荡,可以增强2.18 +/- 0.08年周期伽马射线周期的边际重要性。程序和Swift-UVOT。在类似于10年数据中出现的光周期具有相似的周期,而15 GHz振荡的规律性不如在其他频带中看到的那样。对于这种准星的进一步长期多波长监测可能会在这种准周期的可能解释中有所区别。

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