Non-equilibrium Photoionization and Hydrodynamic Simulations of Starburst-driven Outflows
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The document discusses non-equilibrium photoionization and hydrodynamic simulations related to starburst-driven outflows in galaxies. It covers background theory, hydrodynamic setups, emissivity calculations, and applications to star-forming galaxies, along with future plans for enhancing simulations. Key findings include the effects of cooling on wind formation and proposed advancements in radiative transfer modeling.
![13 Oct 2021 MHD-PP
5
Strong Cooling & Suppressed Winds
NGC 2366
Green Pea analog!
[O II], [O III] and Continuum (Oey+ 2017)
Mrk 71
Oey + 2017](https://image.slidesharecdn.com/2021danehkarmhd-pp-211015212632/85/Non-equilibrium-Photoionization-and-Hydrodynamic-Simulations-of-Starburst-driven-Outflows-5-320.jpg)
Non-equilibrium Photoionization and Hydrodynamic Simulations of Starburst-driven Outflows
- 1. Non-equilibrium Photoionization Non-equilibrium Photoionization and Hydrodynamic Simulations and Hydrodynamic Simulations of Starburst-driven Outflows of Starburst-driven Outflows Starburst-driven Outflow (Romero+ 2018, Strickland+ 2003) Ashkbiz Danehkar Department of Astronomy, University of Michigan danehkar@umich.edu In Collaborations with: Sally Oey, and Will Gray Fourth Virtual Workshop on Numerical Modeling in MHD and Plasma Physics (MHD-PP), October 13, 2021
- 2. 13 Oct 2021 MHD-PP 2 Starburst-driven Outflows Starburst-driven Outflows and Bubbles in NGC 3079 (Credit: X-ray:NASA/CXC/UMich/J-T Li;Optical:NASA/STScI)
- 3. 13 Oct 2021 MHD-PP 3 Starburst-driven Outflows Starburst-driven Outflows (Romero+ 2018, Strickland+ 2003)
- 4. 13 Oct 2021 MHD-PP 4 Outline Background: Starburst-driven Outflows – Adiabatic Wind and Bubble Formation Solutions – Radiative Semi-analytic Wind Solutions Hydrodynamic Setup: NEI Radiative Cooling in FLASH – Radiative Cooling Rates + Photo-Heating Rates Emissivity Calculations: CLOUDY Photoionization Modeling – CIE+PIE Implementation – NEI+PIE Implementation Applications: Star-forming galaxies – Optical BPT and UV Diagnostic Diagrams Future Plans: Detailed Radiative Transfer, 2D Simulations
- 5. 13 Oct 2021 MHD-PP 5 Strong Cooling & Suppressed Winds NGC 2366 Green Pea analog! [O II], [O III] and Continuum (Oey+ 2017) Mrk 71 Oey + 2017
- 6. 13 Oct 2021 MHD-PP 6 Strong Cooling & Suppressed Winds Super Star Cluster NGC 5253 (Turner et al. 2017)
- 7. 13 Oct 2021 MHD-PP 7 Wind Formation: Adiabatic Theory Adiabatic Solutions – Adiabatic Wind (γ=5/3) – Chevalier & Clegg 1985 Chevalier & Clegg 1985
- 8. 13 Oct 2021 MHD-PP 8 Wind Formation: Adiabatic Theory Different Wind Regions, as defined by Weaver+ 1977
- 9. 13 Oct 2021 MHD-PP 9 Wind Formation: Radiative Solution Radiative Semi-analytic Solutions – Silich + 2004 – With Radiative Cooling Silich + 2004
- 10. 13 Oct 2021 MHD-PP 10 Wind Formation: Radiative Solution Radiative Cooling Silich + 2004 Silich + 2004
- 11. 13 Oct 2021 MHD-PP 11 Hydrodynamic Simulations Danehkar, Oey, Gray, 2021
- 12. 13 Oct 2021 MHD-PP 12 Hydrodynamic Simulations Solve using a hybrid Riemann solver (Roe+HLLE) in FLASH – Unsplit Hydrodynamic Solver – 2nd -order MUSCL-Hancock Scheme Coupled with the Non-equilibrium Atomic Chemistry and Cooling Package MAIHEM (Gray + 2019) – Radiative Cooling Function (Λ) – Photo-Heating Function (Γ)
- 13. 13 Oct 2021 MHD-PP 13 Hydrodynamic Simulations Boundary Conditions: Initial Conditions: Radiative Cooling Function (Λ) and Photo-Heating Function (Γ): Included in the Atomic Chemistry and Cooling Package MAIHEM (Gray + 2019)
- 14. 13 Oct 2021 MHD-PP 14 Hydrodynamic Simulations Cooling Function (Λ) and Photo-Heating Function (Γ): Included in the Atomic Chemistry and Cooling Package MAIHEM (Gray + 2019): Cooling Efficiencies from (Λi ) calculated using ion-by-ion efficiencies from Gnat & Ferland 2012. Heating Efficiencies from (Γi ) calculated using photoionization cross sections from Verner & Yakovlev 1995, and Verner, Ferland, et al. 1996.
- 15. 13 Oct 2021 MHD-PP 15 Hydrodynamic Simulations Model Grids: https://superwinds.astro.lsa.umich.edu/ Temperature Density Danehkar, Oey, Gray, 2021
- 16. 13 Oct 2021 MHD-PP 16 Hydrodynamic Simulations Adiabatic Bubble (AB) Catastrophic Cooling Bubble (CB) Catastrophic Cooling (CC) Danehkar, Oey, Gray, 2021
- 17. 13 Oct 2021 MHD-PP 17 Hydrodynamic Simulations Adiabatic Bubble (AB), Catastrophic Cooling Bubble (CB) Catastrophic Cooling (CC), momentum-conserving (MC) Temperature discrepancy factor (fT = Tw / Tadi) Danehkar, Oey, Gray, 2021
- 18. 13 Oct 2021 MHD-PP 18 Hydrodynamic Simulations Adiabatic Bubble (AB), Adiabatic Pressure-Confined (AP) Catastrophic Cooling (CC), Catastrophic Cooling Bubble (CB) Temperature discrepancy factor (fT = Tw / Tadi) Danehkar, Oey, Gray, 2021
- 19. 13 Oct 2021 MHD-PP 19 Danehkar, Oey, Gray, 2021 Hydrodynamic Simulations (Danehkar, Oey, Gray, 2021)
- 20. 13 Oct 2021 MHD-PP 20 Photoionization Modeling (CIE+PIE=CPI) Danehkar, Oey, Gray, 2021 Photoionization + Collisional Ionization
- 21. 13 Oct 2021 MHD-PP 21 Photoionization Modeling (CIE+PIE=CPI) Danehkar, Oey, Gray, 2021 PIE (Pure Photoionization), CIE+PIE=CPI (Photoionization + Collisional Ionization)
- 22. 13 Oct 2021 MHD-PP 22 Photoionization Modeling (NEI+PIE=NPI) Danehkar, Oey, Gray, 2021 Photoionization + Non-equilibrium Ionization
- 23. 13 Oct 2021 MHD-PP 23 Photoionization Modeling (NEI+PIE=NPI) PIE (Pure Photoionization), CIE+PIE=CPI (Photoionization + Collisional Ionization), NEI+PIE=NPI (Photoionization + Non-equilibrium Ionization), Danehkar, Oey, Gray, 2021
- 24. 13 Oct 2021 MHD-PP 24 Optical & UV Diagnostic Diagrams Emission Lines of Superwinds Danehkar, Oey, Gray, 2021
- 25. 13 Oct 2021 MHD-PP 25 Optical BPT Diagrams Danehkar, Oey, Gray, 2021 Optical Emission Lines (radiation-bounded)
- 26. 13 Oct 2021 MHD-PP 26 UV Diagnostic Diagrams Danehkar, Oey, Gray, 2021 UV Emission Lines (radiation-bounded)
- 27. 13 Oct 2021 MHD-PP 27 UV Diagnostic Diagrams UV Emission Lines (radiation-bounded) Danehkar, Oey, Gray, 2021
- 28. 13 Oct 2021 MHD-PP 28 Future Plans: Extension to 2D Allow to Study Different Instabilities Rayleigh-Taylor instability, Richtmyer-Meshkov instability, Kelvin-Helmholtz instability Formation of Instability-induced Dense Clumps Lancaster, Ostriker, et al. 2021
- 29. 13 Oct 2021 MHD-PP 29 Future Plans: Extension to 2D Allow to Study Different Instabilities Rayleigh-Taylor instability, Richtmyer-Meshkov instability, Kelvin-Helmholtz instability Formation of Instability-induced Dense Clumps Lancaster, Ostriker, et al. 2021
- 30. 13 Oct 2021 MHD-PP 30 Future Plans: RT Implementation Implementation of detailed Radiative Transfer (RT) calculations Improvement of radiative cooling and photo-heating processes Stellar flux at a given distance (e.g. Klassen + 2014): Inclusion of radiation pressure: Included in MAIHEM Need RT calculations
- 31. 13 Oct 2021 MHD-PP 31 Concluding Points Starburst-driven Outflows – Adiabatic Solution (Chevalier & Clegg 85) – Radiative Solution (Silich + 2004) Non-equilibrium Cooling Hydrodynamic Simulations – MAIHEM Cooling Package (Gray + 2019): Radiative Cooling + Photo-Heating – Parameter Space Investigation (Danehkar, Oey, Gray, 2021, ApJ, arXiv:2106.10854) Photoionizaion Modeling – CIE+PIE (Danehkar et al. ApJ, 2021; arXiv:2106.10854) – NEI+PIE (Danehkar, et al. in preparation) Future Plans – Detailed Radiative Transfer Implementation: Improved Radiative Solutions – 2-D Simulation: Instability-induced Clumps
- 32. 13 Oct 2021 MHD-PP 32 Thank you for your attention Starburst-driven Outflow (Romero+ 2018, Strickland+ 2003)