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

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arxiv 2110.11900 v1 pith:VZ73GSFT submitted 2021-10-22 astro-ph.GA astro-ph.HE

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

Dipanjan Mukherjee , Geoffrey V. Bicknell , Alexander Y. Wagner This is my paper
classification astro-ph.GA astro-ph.HE
keywords distributiondynamicsformationimplicationsinteractionjetsscalessimulations
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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.

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