Overview
Giant molecular clouds are the cradles of star clusters, in which most stars form, particularly in the early Universe. Understanding the modes and the efficiency with which stars and clusters form remains a central challenge in modern astrophysics.
Simulating clustered star formation in cosmic morning
We develop a continuous star cluster formation model in the cosmological hydrodynamic code ART to simulate the effects of clustered star formation during the Cosmic Dawn on the observational properties of the earliest galaxies by the Hubble and James Webb Space Telescopes. The figure in the left shows sketch of a star-froming cloud in simulations.
