标题： 解析的喷流与星际物质相互作用模拟：对气体动力学和恒星形成的启示 显示英文标题

标题： Resolved simulations of jet-ISM interaction: Implications for gas dynamics and star formation

摘要： 相对论性喷流可以在突破到更大尺度之前与宿主星系的弥漫气体分布相互作用。在过去十年中，有几项研究通过模拟由喷流驱动的外流，来理解它们如何影响近邻环境以及此类相互作用发生的空间和时间尺度。这些模拟能够捕捉喷流与湍动且块状的星际介质之间的相互作用以及气体的能量学结果。在这篇综述中，我们总结了这类近期研究的结果，并讨论了它们对气体分布动力学演化以及恒星形成率的影响。 显示英文摘要

摘要： Relativistic jets can interact with the ambient gas distribution of the host galaxy, before breaking out to larger scales. In the past decade several studies have simulated jet-driven outflows to understand how they affect the nearby environment, and over what spatial and temporal scales such interactions occur. The simulations are able to capture the interaction of the jets with the turbulent clumpy interstellar medium and the resultant energetics of the gas. In this review we summarise the results of such recent studies and discuss their implications on the evolution of the dynamics of the gas distribution and the star formation rate.