Galaxy evolution strongly depends on the physics of the interstellar medium (ISM). The ISM is permeated by magnetic fields (B-fields), in which magnetic energy is in close equipartition with the thermal and kinetic energy. This physical condition makes the B-fields dynamically important at several stages of galaxy evolution, affecting gas flows in

Zoom link: https://rediris.zoom.us/j/93247225390?pwd=RG4xUjh0eDc5Q2hOK3N1T0xPMmQ1d… Meeting ID: 932 4722 5390 Passcode: 551463

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At present, our understanding of the formation history of the MW is limited due to the complexity of observing the imprints of accretion events and of reproducing them in numerical simulations. Moreover, though being the only galaxy, in which the Galactic potential can be probed in detail, the distribution of mass in the MW, and hence of the dark

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