Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …

Giant molecular clouds (GMCs) are the sites of star formation and stellar feedback in
galaxies. Their properties set the initial conditions for star formation and their lifecycles …

We examine the factors responsible for the variation in the ionization parameter (U) of high-
redshift star-forming galaxies based on medium-resolution JWST/NIRSpec observations …

Integral field units enable resolved studies of a large number of star-forming regions across
entire nearby galaxies, providing insight on the conversion of gas into stars and the …

By performing 3D radiation hydrodynamics simulations, we study the formation of young
massive star clusters (YMCs; M*> 104 M⊙) in clouds with the surface density ranging from …

We present a new fried grid of mass-loss rates for externally far-ultraviolet (FUV) irradiated
protoplanetary discs. As a precursor to the new grid, we also explore the microphysics of …

We present simulations of the formation and evolution of clusters in spiral arms. The
simulations follow two different spiral arm regions, and the total gas mass is varied to …

We couple star cluster formation and feedback simulations of a Carina-like star-forming
region with 1D disc evolutionary models to study the impact of external photoevaporation on …

ABSTRACT The Galactic Centre is known to have undergone a recent star formation
episode a few Myr ago, which likely produced many T Tauri stars hosting circumstellar discs …

We have performed simulations of cluster formation along two regions of a spiral arm taken
from a global Milky Way simulation, including photoionizing feedback. One region is …