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...
With more than 4000 exoplanets found and about 2-dozens of planets with detected atmospheric chemical species, we moved from an era of discovery to a new era of exoplanet characterisation. On the othe...
Supernovae (SNe) are one of the most energetic explosion events in the universe, with the human detectability not only in electromagnetic waves but also neutrino and possibly gravitational waves. They...
Cosmic rays (CRs) is one of the most important component in the interstellar medium (ISM) in our Galaxy. The high energy CRs will interact with the ambient gas and produce gamma-rays, which dominate t...
Atmospheric escape is an important process in the evolution of exoplanet atmospheres, especially those orbiting very close to their host stars. However, many aspects of atmospheric escape remain poorl...
Despite tremendous recent progress, gaps remain in our knowledge of our cosmic history. For example, we have yet to make direct observations of Cosmic Dawn or the subsequent Epoch of Reionization. Tog...