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A Review of the Theory of Galactic Winds Driven by Stellar Feedback

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arxiv 1811.00558 v1 pith:Q46PSTKN submitted 2018-11-01 astro-ph.GA

Dong Zhang This is my paper · ORCID
classification astro-ph.GA
keywords windsgalacticreviewstellarassociateddrivenfeedbackformation
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Galactic winds from star-forming galaxies are crucial to the process of galaxy formation and evolution, regulating star formation, shaping the stellar mass function and the mass-metallicity relation, and enriching the intergalactic medium with metals. Galactic winds associated with stellar feedback may be driven by overlapping supernova explosions, radiation pressure of starlight on dust grains, and cosmic rays. Galactic winds are multiphase, the growing observations of emission and absorption of cold molecular, cool atomic, ionized warm and hot outflowing gas in a large number of galaxies have not been completely understood. In this review article, I summarize the possible mechanisms associated with stars to launch galactic winds, and review the multidimensional hydrodynamic, radiation hydrodynamic and magnetohydrodynamic simulations of winds based on various algorithms. I also briefly discuss the theoretical challenges and possible future research directions.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. JWST absorption line spectroscopy with SPURS: ISM covering fractions and kinematics in individual galaxies at $z=5-9$

    astro-ph.GA 2026-06 unverdicted novelty 7.0 of 10

    JWST spectra of six z=5-9 galaxies show low-ionization covering fractions of 0.2-0.9 and diverse kinematics including blueshifted outflows, indicating heterogeneous multiphase ISM.

  2. Unveiling Metal Mixing in a Grand-Design Spiral: A UV-optical multiphase spatially resolved study of M83

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    Multiphase abundance mapping of M83 reveals a persistent roughly 1.5 dex nitrogen excess in ionized gas relative to neutral gas around young clusters, indicating slow metal mixing in a massive spiral.

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