Stellar jets are narrow streams of gas and dust ejected from young stars during their formation process. These jets are typically highly collimated and can extend over large distances in space. Stellar jets are believed to be formed as a result of the star's magnetic field interacting with the surrounding material in the star-forming region, causing the material to be ejected along the magnetic field lines. Stellar jets play a crucial role in shaping the surrounding interstellar medium and are thought to influence the formation of planets and other objects in the star's planetary system. Studying stellar jets can provide valuable insights into the processes involved in star formation and the dynamics of young stars. Observational studies of stellar jets involve using telescopes and other instrumentation to study the emission and structure of the jets in various wavelengths, such as visible light, infrared, and radio waves. Theoretical studies also aim to model the physical processes that govern the formation and evolution of stellar jets. Overall, research on stellar jets helps to deepen our understanding of the complex processes involved in the birth of stars and planetary systems.