在河外天体的光谱中发现的高度特殊的发射谱线可能是由超快速准周期振荡产生的

E. Borra
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引用次数: 0

摘要

在一些活动星系核和类星体的光谱中发现了极其特殊的发射线。它们的起源是完全未知的。我们研究了一种假设,即它们是由射流或黑洞中可能发生的超快速准周期振荡产生的,正如一篇发表的理论论文所预测的那样。我们的结论是,虽然不能完全确定,但这个假设与之前提出的其他非常奇特的假设(例如,由于接近光速的物体运动而产生的蓝移)一样有效。我们考虑进一步验证我们假设的方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Highly Peculiar Emission lines detected in Spectra of Extragalactic objects may be generated by Ultra-rapid Quasi-periodic Oscillations
Extremely peculiar emission lines have been found in the spectra of some active galactic nuclei and quasars. Their origin is totally unknown. We investigate the hypothesis that they are generated from ultra-rapid quasi-periodic oscillations that may occur in jets or black holes, as predicted in a published theoretical paper. We conclude that, although not totally certain, this hypothesis is just as valid as the other highly peculiar hypotheses that have been previously made (e.g. blueshifts due to bulk motions close to the speed of light). We consider ways to further validate our hypothesis.
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