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Bilateral symmetry in active galaxies [Review]

机译:活跃星系中的双边对称性[综述]

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The bilateral symmetry around active galaxies was discovered in the radio continuum in the 1950s. It has since been found to manifest itself throughout the electromagnetic spectrum in the continuum as well as lines, on scales from subparsec to megaparsecs. Detailed observations have often led to classification schemes based on different length- and time-scales, and types and stages of activity. Consolidation of continuum and line observations in total and polarized intensities in various bands of the electromagnetic spectrum from gamma-rays to radio should lead to a more complete picture, unifying these schemes into a physical whole. We review these observations of active galaxies and their current models, and how well the two fit together. Our emphasis throughout is on bilateral structure in and around active galaxies. (C) 1998 Elsevier Science B.V. All rights reserved. [References: 582]
机译:在1950年代的连续射电中发现了活跃星系周围的双侧对称性。从那以后,人们发现它在整个电磁谱中都表现出连续性和线性,范围从次等到大等。详细的观察常常导致基于不同长度和时间尺度以及活动类型和阶段的分类方案。合并从伽马射线到无线电波的电磁频谱各个波段中的总强度和极化强度的连续谱和线谱观测结果,应该会得到更完整的图像,将这些方案统一为一个物理整体。我们回顾了对活动星系及其当前模型的观察,以及两者的融合程度。我们整个过程的重点是活跃星系及其周围的双边结构。 (C)1998 Elsevier Science B.V.保留所有权利。 [参考:582]

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