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

Dipanjan Mukherjee; Geoffrey V. Bicknell; Alexander Y. Wagner

doi:10.1002/asna.20210061

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

Dipanjan Mukherjee^*, Geoffrey V. Bicknell, Alexander Y. Wagner

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

18 Citations (Scopus)

Abstract

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 summarize 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.

Original language	English
Pages (from-to)	1140-1145
Number of pages	6
Journal	Astronomische Nachrichten
Volume	342
Issue number	9-10
DOIs	https://doi.org/10.1002/asna.20210061
Publication status	Published - 1 Nov 2021

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10.1002/asna.20210061

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abstract = "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 summarize 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.",

author = "Dipanjan Mukherjee and Bicknell, \{Geoffrey V.\} and Wagner, \{Alexander Y.\}",

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AU - Bicknell, Geoffrey V.

AU - Wagner, Alexander Y.

PY - 2021/11/1

Y1 - 2021/11/1

N2 - 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 summarize 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.

AB - 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 summarize 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.

UR - https://www.scopus.com/pages/publications/85119270878

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DO - 10.1002/asna.20210061

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JO - Astronomische Nachrichten

JF - Astronomische Nachrichten

IS - 9-10

ER -

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

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