Star Formation and Evolution

Star formation is the process by which dense regions in clouds of gas and dust collapse under gravity, leading to the birth of stars. In computational astrophysics, scientists use simulations to model these dynamic processes, including the heating, cooling, and chemical reactions that occur as material condenses. As a star evolves, it undergoes changes, moving through various stages like main sequence, red giant, and eventually ending as a white dwarf, neutron star, or black hole. These simulations help us understand not only star life cycles but also how they influence galaxies and the universe's evolution.