▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density
regimes in the interstellar gas. This two-part review summarizes the observations, theory …

This review examines observations of magnetic fields in molecular clouds and what those
observations tell us about the theory of molecular cloud evolution and star formation. First …

Cold dark clouds are nearby members of the densest and coldest phase in the Galactic
interstellar medium, and represent the most accessible sites where stars like our Sun are …

Recent studies of the nearest star-forming clouds of the Galaxy at submillimeter wavelengths
with the Herschel Space Observatory have provided us with unprecedented images of the …

Our current understanding of the physical processes of star formation is reviewed, with
emphasis on processes occurring in molecular clouds like those observed nearby. The …

We report high-angular-resolution measurements of polarized dust emission toward the low-
mass protostellar system NGC 1333 IRAS 4A. We show that in this system the observed …

ABSTRACT A key uncertainty in galaxy evolution is the physics regulating star formation,
ranging from small-scale processes related to the life-cycle of molecular clouds within …

We describe a morphological imprint of magnetization found when considering the relative
orientation of the magnetic field direction with respect to the density structures in simulated …

Dust coagulation in dense molecular clouds: The formation of fluffy aggregates ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …

We study the equilibrium of pressure truncated, filamentary molecular clouds that are
threaded by rather general helical magnetic fields. We first apply the virial theorem to …