We present observational evidence of a correlation between the high-mass slope of the
stellar initial mass function (IMF) in young star clusters and their stellar surface density, σ …

Using the optimal sampling model, we synthesized the embedded clusters of ATLASGAL
clumps with H ii regions (H ii-clumps). The 0.1 Myr isochrone was used to estimate the …

Abstract 1226 ATLASGAL clumps with H ii regions (H ii-clumps) were matched with radio
sources in the CORNISH-North/South surveys, and 392 of them have corresponding radio …

We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum
survey of almost half of the Galactic Plane (251°≤ l≤ 358° and 2°≤ l≤ 61° at| b|≤) …

We present a comparison of the Milky Way's star formation rate (SFR) surface density (∑
SFR) obtained with two independent state-of-the-art observational methods. The first method …

Stellar feedback influences the star formation rate (SFR) and the interstellar medium of
galaxies in ways that are difficult to quantify numerically, because feedback is an essential …

Hub-filament systems (HFSs) are potential sites of massive star formation (MSF). To
understand the role of filaments in MSF and the origin of HFSs, we conducted a multiscale …

In the article, a method is developed for estimating the dynamic masses of the stellar and
gas components of cluster-cloud systems under conditions of non-isolation and significant …

We present the SARAO MeerKAT Galactic Plane Surv ey (SMGPS), a 1.3 GHz continuum
surv ey of almost half of the Galactic Plane (251◦≤ l≤ 358◦ and 2◦≤ l≤ 61◦ at| b|≤ 1.◦ 5) …

The star formation rate (SFR) of the Milky Way is poorly understood in comparison to the
SFR of other galaxies. In order to better find the Galaxy's place in the universe, it is …