INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars

The formation and evolution of galaxies have proved sensitive to the inclusion stellar feedback, which is therefore crucial any successful galaxy model. We present INFERNO, a new model for hydrodynamic simulations galaxies, incorporates resolved objects with star-by-star calculations when where injection enriched material, momentum, energy takes place. INFERNO treats early kinematics include phenomena such as walkaway runaway stars. employ this innovative on dwarf demonstrate that our physically motivated feedback can drive vigorous galactic winds. This quantified by mass metal loading factors in range $10-100$, an factor close unity. Outflows are established disc, highly multi-phase, spanning almost $8$ orders magnitude temperature, clear dichotomy between ejected cold, slow-moving ($T\lesssim5\times10^4\,{\rm K}$, $v<100\,{\rm km\,s}^{-1}$) gas hot, fast-moving ($T>10^6\,{\rm $v>100\,{\rm gas. In contrast massive disc we find surprisingly weak impact kinematics, stars having little no effect results, despite exploding diffuse outside dense star-forming gas, well entirely. stems from combination strong porous interstellar medium, obscure unique signatures provide.