The inner∼ 200 pc region of the Galaxy contains a 4 million M⊙ supermassive black hole
(SMBH), significant quantities of molecular gas, and star formation and cosmic-ray energy …

Context. While star formation on large molecular cloud scales and on small core and disk
scales has been investigated intensely over the past decades, the connection of the large …

Galactic plane radio surveys play a key role in improving our understanding of a wide range
of astrophysical phenomena. Performing such a survey using the latest interferometric …

Context. Cygnus X is one of the closest and most active high-mass star-forming regions in
our Galaxy, making it one of the best laboratories for studying massive star formation. Aims …

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 …

Studies of Galactic H II regions are of crucial importance for studying star formation and the
evolution of the interstellar medium. Gaining an insight into their physical characteristics …

Context. The properties of the population of Galactic supernova remnants (SNRs) are
essential to our understanding of the dynamics of the interstellar medium (ISM) in the Milky …

We present new continuum and molecular line data from the ALMA Three-millimeter
Observations of Massive Star-forming regions (ATOMS) survey for the two protoclusters …

As part of the Global View on Star Formation (GLOSTAR) survey we have used the Karl G.
Jansky Very Large Array (VLA) in its B-configuration to observe the part of the Galactic plane …

Context. Diffuse interstellar bands (DIBs) are common interstellar absorption features in
spectroscopic observations but their origins remain unclear. DIBs play an important role in …