Classical quasar winds, which are gas outflows from the accretion disks surrounding supermassive black holes, play a crucial role in regulating the coevolution between the black hole and its host galaxy (Kormendy & Ho 2013). These outflows are also believed to contribute to the observed correlations between the black hole mass and the properties of the surrounding bulge (Ferrarese & Merritt 2000; Gebhardt et al. 2000). Additionally, quasar outflows have been proposed as potential mechanisms for active galactic nuclei feedback processes, including the termination of star formation in the interstellar medium and the regulation of accretion onto the black hole (Fabian 2012; King & Pounds 2015). (78 words

阅读以下文段写3句关于类星体外流的英文简介作为相关研究的引言的开头保留括号里的参考文献:Outflowswinds are a significant component of the quasar phenomenon and are plausible candidates for regulating potential coevolution between the central sup

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