High-Energy Astronomy

High-energy astronomy studies astronomical phenomena that emit radiation at high energies, such as X-rays and gamma-rays. This field focuses on extreme environments like black holes, neutron stars, supernovae, and active galaxies, where matter is heated to millions of degrees or accelerated to near light speeds. By observing these energetic emissions, scientists can uncover the processes governing the universe's most violent and dynamic events. Understanding high-energy sources helps us learn about the life cycles of stars, the structure of galaxies, and the fundamental laws of physics that govern the cosmos, providing critical insights into galactic evolution and cosmic history.