  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.
