We combine previously published interferometric and single-dish data of relatively nearby
massive dense cores that are actively forming stars to test whether their 'fragmentation …

In the star-formation process, the vital impact of environmental factors such as feedback from
massive stars and stellar density on the form of the initial mass function (IMF) at the low …

Context. Through observations numerous giant molecular filaments (GMFs) have been
discovered in the Milky Way. Their role in the Galactic star formation and Galaxy-scale …

Hierarchical Fragmentation in the Perseus Molecular Cloud: From the Cloud Scale to
Protostellar Objects - IOPscience This site uses cookies. By continuing to use this site you agree …

We present subarcsecond 1.3 mm continuum ALMA observations toward the Orion
Molecular Cloud 1 South (OMC-1S) region, down to a spatial resolution of 74 au, which …

We present an analysis of multi-wavelength observations from various data sets and
Galactic plane surveys to study the star-formation process in the W42 complex. A bipolar …

One of the key questions in the field of star formation is the role of stellar feedback on the
subsequent star formation process. The W3 giant molecular cloud complex at the western …

The structure of molecular clouds holds important clues regarding the physical processes
that lead to their formation and subsequent dynamical evolution. While it is well established …

Context. Molecular clouds trace the spiral arms of the Milky Way and all its star forming
regions. Large-scale mapping of molecular clouds will provide an approach to understand …

W4 is a giant H ii region ionized by the OB stars of the cluster IC 1805. The H ii region/cluster
complex has been a subject of numerous investigations as it is an excellent laboratory for …