<p>Over the past decades, the discovery of a large number of young massive clusters (YMCs) in the local Universe and giant clumps in high-z galaxies suggests that clustered star formation is the dominant...</p>
Galaxy formation is an essential research area in astronomy. In recent years, high-resolution cosmological zoom-in simulations with realistic multi-phase ISM, star formation, and feedback models have ...
The search for extrasolar planets initially focused on Sun-like FGK main-sequence stars, but efforts have been made in recent years to search for planets around more massive stars in their giant phase...
Fast radio bursts (FRBs) are millisecond radio pulses detected from cosmological distances. A large number of models invoke extragalactic magnetars as the sources of these mysterious events. Magnetars...
Recent ground based observations at various wavelengths reveal a variety of protoplanetary disk structures. These disk structures may help us to constrain the planet formation process. We apply the pl...
The study of GRBs has been an active field in astrophysics over the years, which has undergone a significant boost in interest with the joint detection of GW170817/GRB 170817A and several new types of...
Planets form from discs of material around young (oduced in clusters. There is a growing realisation that planet-forming discs are not isolated systems and instead are influenced by the gravitational ...
Kinetic field theory (KFT) has been developed in recent years to study structure formation in ensembles of classical particles in and out of equilibrium. In a straightforward manner, KFT can be specia...
Quenched massive spiral galaxies have attracted great attention recently, as more data is available to constrain their environment and cold gas content. However, the quenching mechanism is still uncer...
Recent spatially-resolved studies have suggested that some of the correlations among global quantities (e.g., star formation rate, stellar mass, gas mass) might be an ensemble effect of local processe...