Star-forming regions are areas within galaxies where new stars are being born. These regions are characterized by large concentrations of gas and dust, which are the raw materials from which stars are formed. The process of star formation typically begins when these materials are compressed and heated, causing them to collapse under their own gravity and eventually form into protostars. These protostars continue to grow in mass and eventually reach a point where nuclear fusion reactions begin, marking the official birth of a new star. Studying star-forming regions provides valuable insights into the formation and evolution of stars, as well as the processes that govern the formation of galaxies as a whole.