Star Formation
Star formation refers to the process by which dense regions within molecular clouds in space, composed of gas and dust, collapse under their own gravity to form new stars. This process is influenced by various factors such as temperature, pressure, magnetic fields, and rotation. The study of star formation is a key area of research in astrophysics, as it provides insights into the origins of stars, planetary systems, and the elements that make up the universe. It is closely related to other areas of astronomy and astrophysics, such as the interstellar medium, stellar evolution, and cosmology. Star formation is a complex and dynamic process that involves a range of physical phenomena, from the smallest scales of individual atoms and molecules to the largest scales of galaxies and galaxy clusters.