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Galaxies appear simpler than expected

机译:星系似乎比预期的简单

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摘要

Galaxies are complex systems the evolution of which apparently results fromthe interplay of dynamics, star formation, chemical enrichment, and feedbackfrom supernova explosions and supermassive black holes. The hierarchical theoryof galaxy formation holds that galaxies are assembled from smaller pieces,through numerous mergers of cold dark matter. The properties of an individualgalaxy should be controlled by six independent parameters including mass,angular-momentum, baryon-fraction, age and size, as well as by the accidents ofits recent haphazard merger history. Here we report that a sample of galaxiesthat were first detected through their neutral hydrogen radio-frequencyemission, and are thus free of optical selection effects, shows fiveindependent correlations among six independent observables, despite having awide range of properties. This implies that the structure of these galaxiesmust be controlled by a single parameter, although we cannot identify thisparameter from our dataset. Such a degree of organisation appears to be at oddswith hierarchical galaxy formation, a central tenet of the cold dark matterparadigm in cosmology.
机译:星系是复杂的系统,其演化显然是由动力学,恒星形成,化学富集以及超新星爆炸和超大质量黑洞的反馈相互作用所致。星系形成的分层理论认为,星系是通过冷暗物质的多次合并而由较小的碎片组装而成的。单个星系的属性应通过六个独立的参数进行控制,包括质量,角动量,重子分数,年龄和大小以及最近的偶然合并历史的意外事件。在这里,我们报告说,一个样本星系首先通过其中性氢射频发射被发现,因此没有光学选择效应,尽管具有广泛的特性范围,但它们显示了六个独立可观测物之间的五个独立相关性。这意味着这些星系的结构必须由单个参数控制,尽管我们无法从数据集中识别出该参数。这样的组织程度似乎与宇宙星系中冷暗物质范式的中心原理-等级星系形成不一致。

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