Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

The discovery of large numbers of young low-mass stars and brown dwarfs over the past
decade has made it possible to investigate star formation and early evolution in a previously …

We determine the observational signatures of protostellar cores by coupling two-
dimensional radiative transfer calculations with numerical hydrodynamical simulations that …

Abstract attempted to derive the stellar initial mass function (IMF) as a consequence of
lognormal density fluctuations in a turbulent medium, using an argument similar to for …

Abstract We present the Atacama Large Millimeter/submillimeter Array survey of CO (2–1)
emission from the 1/5 solar metallicity, Local Group dwarf galaxy NGC 6822. We achieve …

We investigate the roles of magnetic fields and ambipolar diffusion during prestellar core
formation in turbulent giant molecular clouds, using three-dimensional numerical …

The fragmentation of star-forming interstellar clouds, and the resulting stellar initial mass
function (IMF), is strongly affected by the temperature structure of the collapsing gas. Since …

We investigate protostellar outflow evolution, gas entrainment, and star formation efficiency
using radiation-hydrodynamic simulations of isolated, turbulent low-mass cores. We adopt …

We use numerical hydrodynamic simulations to investigate prestellar core formation in the
dynamic environment of giant molecular clouds, focusing on planar post-shock layers …

Abstract We present QUI JOint TEnerife (QUIJOTE) intensity and polarisation maps at 10–20
GHz covering a region along the Galactic plane 24°≲ l≲ 45°,| b|≲ 8°. These maps result …