The Structure of Multiphase Galactic Winds
arXiv:2108.05355 · doi:10.3847/1538-4357/ac2f41
Abstract
We present a novel analytic framework to model the steady-state structure of multiphase galactic winds comprised of a hot, volume-filling component and a cold, clumpy component. We first derive general expressions for the structure of the hot phase for arbitrary mass, momentum, and energy sources terms. Next, informed by recent simulations, we parameterize the cloud-wind mass transfer rates, which are set by the competition between turbulent mixing and radiative cooling. This enables us to cast the cloud-wind interaction as a source term for the hot phase and thereby simultaneously solve for the evolution of both phases fully accounting for their bidirectional influence. With this model, we explore the nature of galactic winds over a broad range of conditions. We find that: (i) with realistic parameter choices, we naturally produce a hot, low-density wind that transports energy while entraining a significant flux of cold clouds, (ii) mixing dominates the cold cloud acceleration and decelerates the hot wind, (iii) during mixing thermalization of relative kinetic energy provides significant heating, (iv) systems with low hot-phase mass loading factors and/or star formation rates can sustain higher initial cold phase mass loading factors, but the clouds are quickly shredded, and (v) systems with large hot-phase mass loading factors and/or star formation rates cannot sustain large initial cold-phase mass loading factors, but the clouds tend to grow with radius. Our results highlight the necessity of accounting for the multiphase structure of galactic winds, both physically and observationally, and have important implications for feedback in galactic systems.
41 pages, 11 figures, submitted to ApJ. Schematic overview shown in Fig. 1 available at https://dfielding14.github.io/images/Multiphase_Winds_Schematic.pdf . Example code available at https://github.com/dfielding14/MultiphaseGalacticWind
References in corpus (55)
- Array Programming with NumPy
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
- Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z=1.4
- The COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-Redshift Circumgalactic Medium
- Mass, Metal, and Energy Feedback in Cosmological Simulations
- Moving mesh cosmology: tracing cosmological gas accretion
- CMasher: Scientific colormaps for making accessible, informative and 'cmashing' plots
- Turbulent Structure of a Stratified Supernova-Driven Interstellar Medium
- The COS-Halos Survey: Metallicities in the Low-Redshift Circumgalactic Medium
- Draping of Cluster Magnetic Fields over Bullets and Bubbles -- Morphology and Dynamic Effects
- Magnetized Gas Clouds can Survive Acceleration by a Hot Wind
- The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling
- Resolving small-scale cold circumgalactic gas in TNG50
- Vertical structure of a supernova-driven turbulent magnetized ISM
- Superbubbles in the Multiphase ISM and the Loading of Galactic Winds
- Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
- Hydrodynamical Coupling of Mass and Momentum in Multiphase Galactic Winds
- Efficiency of gas cooling and accretion at the disc-corona interface
- First results from SMAUG: Characterization of Multiphase Galactic Outflows from a Suite of Local Star-Forming Galactic Disk Simulations
- Dense Molecular Gas Tracers in the Outflow of the Starburst Galaxy NGC 253
- Predictions for the Angular Dependence of Gas Mass Flow Rate and Metallicity in the Circumgalactic Medium
- A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy
- Survival and mass growth of cold gas in a turbulent, multiphase medium
- The extent of chemically enriched gas around star-forming dwarf galaxies
- Growth and structure of multiphase gas in the cloud-crushing problem with cooling
- COS-Burst: Observations of the Impact of Starburst-Driven Winds on the Properties of the Circum-Galactic Medium
- MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a MgII emission halo probed by a quasar sightline
- A Framework for Multiphase Galactic Wind Launching using TIGRESS
- It's Cloud's Illusions I Recall: Mixing Drives the Acceleration of Clouds from Ram Pressure Stripped Galaxies
- A simple model for mixing and cooling in cloud-wind interactions
- HST/STIS spectroscopy of the environment in the starburst core of M82
- The Survival of Multiphase Dusty Clouds in Hot Winds
- Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
- Shock-multicloud interactions in galactic outflows -- II. Radiative fractal clouds and cold gas thermodynamics
- The Physics of Galactic Winds Driven by Cosmic Rays I: Diffusion
- The Physics of Galactic Winds Driven by Cosmic Rays II: Isothermal Streaming Solutions
- The cold circumgalactic medium in emission: MgII halos in TNG50
- The DUVET Survey: Direct -based metallicity mapping of metal-enriched outflows and metal-poor inflows in Mrk 1486
- The Launching of Cold Clouds by Galaxy Outflows. IV. Cosmic-Ray-Driven Acceleration
- Feeding the fire: Tracing the mass-loading of 10^7 K galactic outflows with O VI absorption
- Mapping Outflowing Gas in the Fermi Bubbles: a UV Absorption Survey of the Galactic Nuclear Wind
- The in situ formation of molecular and warm ionised gas triggered by hot outflows
- Cool circumgalactic gas of passive galaxies from cosmological inflow
- A Model for Line Absorption and Emission from Turbulent Mixing Layers
- ALMA Imaging of a Galactic Molecular Outflow in NGC4945
- A 60-kpc Galactic Wind Cone in NGC 3079
- NOEMA High Fidelity Imaging of the Molecular Gas in and around M82
- Thermal Instability and Multiphase Gas in the Simulated Interstellar Medium with Conduction, Viscosity and Magnetic Fields
- Most of the cool CGM of star-forming galaxies is not produced by supernova feedback
- Simulating Gas Inflow at the Disk-Halo Interface
- Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
- Role of cosmic rays in the early stages of galactic outflows
- A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
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- The THESAN project: ionizing escape fractions of reionization-era galaxies
- CLASSY III: The Properties of Starburst-Driven Warm Ionized Outflows
- Bursting Bubbles: Feedback from Clustered SNe and the Trade-off Between Turbulence and Outflows
- Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
- Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
- Radiative turbulent mixing layers at high Mach numbers
- The Circumgalactic Medium of Extreme Emission Line Galaxies at z ~ 2: Resolved Spectroscopy and Radiative Transfer Modeling of Spatially Extended Lyman-alpha Emission in the KBSS-KCWI Survey
- [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
- ALMA Imaging of a Galactic Molecular Outflow in NGC4945
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- The observable properties of cool winds from galaxies, AGN, and star clusters -- II. 3D models for the multiphase wind of M82
- Astraeus VIII: A new framework for Lyman- emitters applied to different reionisation scenarios
- The Anatomy of a Turbulent Radiative Mixing Layer: Insights from an Analytic Model with Turbulent Conduction and Viscosity
- DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy
- Testing SALT Approximations with Numerical Radiation Transfer Code Part 1: Validity and Applicability
- Molecular Shattering
- The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
- Mass-Loading and Non-Spherical Divergence in Hot Galactic Winds: Implications for X-ray Observations