Aims. Surveys of the Milky Way at various wavelengths have changed our view of star
formation in our Galaxy considerably in recent years. In this paper we give an overview of …

Filamentary structures are ubiquitous in high-mass star-forming molecular clouds. Their
relation with high-mass star formation is still to be understood. Here we report interferometric …

The ATOMS, standing for ALMA Three-millimeter Observations of Massive Star-forming
regions, survey has observed 146 active star-forming regions with ALMA band 3, aiming to …

Class II methanol (CH 3 OH) masers are amongst the clearest signposts of recent high-mass
star formation (HMSF). A complete catalogue outlines the distribution of star formation in the …

Magnetic field plays a crucial role in shaping molecular clouds and regulating star formation,
yet the complete information on the magnetic field is not well constrained owing to the …

The latest generation of high-angular-resolution unbiased Galactic plane surveys in
molecular-gas tracers are enabling the interiors of molecular clouds to be studied across a …

The growing range of automated algorithms for the identification of molecular clouds and
clumps in large observational data sets has prompted the need for the direct comparison of …

As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop
a greater understanding for the complex relationships between the large-scale diffuse gas …

The initial physical conditions of high-mass stars and protoclusters remain poorly
characterized. To this end, we present the first targeted ALMA Band 6 1.3 mm continuum …

ABSTRACT The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic
Interstellar Medium) survey used the APEX telescope to map 84 deg2 of the Galactic plane …