银河系:一个活跃的星系?

Back to the Galaxy Pub Date : 2008-05-29 DOI:10.1063/1.43950

W. C. Oelfke

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引用次数: 0

摘要

描述了星系核心的质量密度环境中一个或多个核心黑洞的行为和相互作用，并将这种环境与活动星系典型的大型球形恒星系统的环境进行了比较。本研究提供了局部星系团中一系列星系类型的数据，这些数据表明，在银河系发展的早期阶段，星系核心中坍缩物体或物体系统的动能大于1055尔格的喷射可能发生过，但在后来的时代不太可能发生。

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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The Milky Way: An active galaxy?

The behavior and interactions of one or more core black holes is described for the mass density environment of the galaxy core and comparisons made between this environment and that of a large spherical stellar system typical of an active galaxy. Data is presented for a range of galaxy types in local galaxy clusters that indicates jetting with kinetic energy greater than 1055 ergs from a collapsed object or system of objects in the galaxy core may have occurred during the very early phase of development of the Milky Way but is unlikely in later epochs.

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Back to the Galaxy

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