Resolved simulations of jet-ISM interaction: Implications for gas dynamics and star formation. (arXiv:2110.11900v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Mukherjee_D/0/1/0/all/0/1">Dipanjan Mukherjee</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bicknell_G/0/1/0/all/0/1">Geoffrey V. Bicknell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Wagner_A/0/1/0/all/0/1">Alexander Y. Wagner</a>
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.
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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