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arXiv · 2302.09165

Hydrodynamic Simulations and Time-dependent Photoionization Modeling of Starburst-driven Superwinds

A. Danehkar·M. S. Oey·W. J. Gray
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Abstract

Thermal energies deposited by OB stellar clusters in starburst galaxies lead to the formation of galactic superwinds. Multi-wavelength observations of starburst-driven superwinds pointed at complex thermal and ionization structures which cannot adequately be explained by simple adiabatic assumptions. In this study, we perform hydrodynamic simulations of a fluid model coupled to radiative cooling functions, and generate time-dependent non-equilibrium photoionization models to predict physical conditions and ionization structures of superwinds using the MAIHEM atomic and cooling package built on the program FLASH. Time-dependent ionization states and physical conditions produced by our simulations are used to calculate the emission lines of superwinds for various parameters, which allow us to explore implications of non-equilibrium ionization for starburst regions with potential radiative cooling.

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A. Danehkar, M. S. Oey, W. J. Gray. 2023-02-17. Hydrodynamic Simulations and Time-dependent Photoionization Modeling of Starburst-driven Superwinds. https://doi.org/10.1017/s1743921322001570

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