The relation between Simulated Multiwavelength Blazar Variability and Stochastic Fluctuations

Hannes Thiersen, Michael Zacharias, Markus Böttcher
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Abstract

Blazars exhibit multiwavelength variability, a phenomenon whose underlying mechanisms remain elusive. This study investigates the origin of such variability through leptonic blazar emission simulations, focusing on stochastic fluctuations in environmental parameters. By analyzing the spectral indices of the power spectral densities of the variability, we assess their relationship with the underlying fluctuations. Our findings reveal that the variability spectral indices remain almost independent of the variations responsible for their emergence. This suggests a complex interplay of factors contributing to the observed multiwavelength variability in blazars.
模拟多波长亮星变化率与随机波动之间的关系
耀斑星表现出多波长变异性,这一现象的内在机制仍然难以捉摸。本研究通过对轻子类炽星发射模拟来研究这种变异性的起源,重点是环境参数的随机波动。通过分析变率功率谱密度的谱指数,我们评估了它们与潜在波动的关系。我们的研究结果表明,变异性频谱指数几乎与导致其出现的变异无关。这表明,导致观测到的类星体多波长变率的因素之间存在着复杂的相互作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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