Recent millimeter/submillimeter facilities have revealed the physical properties of
filamentary molecular clouds in relation to high-mass star formation. A uniform survey of the …

Protostellar outflows are one of the most outstanding features of star formation.
Observational studies over the last several decades have successfully demonstrated that …

The nature of molecular clouds and their statistical behavior in subsolar metallicity
environments are not fully explored yet. We analyzed data from an unbiased CO (J= 2–1) …

We have analyzed the data from a large-scale CO survey toward the northern region of the
Small Magellanic Cloud (SMC) obtained with the Atacama Compact Array (ACA) stand …

Low-mass stars are the most numerous stellar objects in the Universe. Before the James
Webb Space Telescope (JWST), we had limited knowledge of how planetary systems …

We investigate the internal kinematics of the young star-forming region NGC 346 in the
Small Magellanic Cloud (SMC). We used two epochs of deep F555W and F814W Hubble …

We present the stellar radial velocity analysis of the central $1^{\prime}\times 1^{\prime} $ of
the young massive Small Magellanic Cloud star cluster NGC 346. Using VLT/MUSE integral …

Collisions between giant molecular clouds (GMCs) are one of the pathways for massive star
formation due to the high densities created. However, the enhancement of the star formation …

Hub-filament systems are considered as natural sites for high-mass star formation.
Kinematic analysis of the surroundings of hub-filaments is essential to better understand …

The NGC 346 young stellar system and associated N66 giant H ii region in the Small
Magellanic Cloud are the nearest example of a massive star-forming event in a low …