English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Thermal energies deposited by OB stellar clusters in starburst galaxies leadto the formation of galactic superwinds. Multi-wavelength observations ofstarburst-driven superwinds pointed at complex thermal and ionizationstructures which cannot adequately be explained by simple adiabaticassumptions. In this study, we perform hydrodynamic simulations of a fluidmodel coupled to radiative cooling functions, and generate time-dependentnon-equilibrium photoionization models to predict physical conditions andionization structures of superwinds using the MAIHEM atomic and cooling packagebuilt on the program FLASH. Time-dependent ionization states and physicalconditions produced by our simulations are used to calculate the emission linesof superwinds for various parameters, which allow us to explore implications ofnon-equilibrium ionization for starburst regions with potential radiativecooling.

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