We review the role that magnetic field may have on the formation and evolution of molecular
clouds. After a brief presentation and main assumptions leading to ideal MHD equations …

In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …

We present a study of the relative orientation between the magnetic field projected onto the
plane of sky (B⊥) on scales down to 0.4 pc, inferred from the polarized thermal emission of …

We use spherically symmetric hydrodynamic simulations to study the dynamical evolution
and internal structure of superbubbles (SBs) driven by clustered supernovae (SNe), focusing …

We statistically evaluated the relative orientation between gas column density structures,
inferred from Herschel submillimetre observations, and the magnetic field projected on the …

Large-scale synchrotron loops are recognized as the main source of diffuse radio-continuum
emission in the Galaxy at intermediate and high Galactic latitudes, yet their origin remain …

We compare the magnetic field orientation for the young giant molecular cloud Vela C
inferred from 500 μm polarization maps made with the BLASTPol balloon-borne polarimeter …

We study the H ii regions associated with the NGC 6334 molecular cloud observed in the
submillimeter and taken as part of the B-fields In STar-forming Region Observations Survey …

Many studies concluded that magnetic fields suppress star formation in molecular clouds
and Milky Way like galaxies. However, most of these studies are based on fully developed …

Massive stellar clusters inject significant mass and energy into their surroundings driving
superbubbles, 100–1000 pc diameter shells of swept-up interstellar material that contain a …