Abstract
Satisfactory assessments of star forming regions in the Galaxy are essential for the understanding of early stellar evolution and today a vast amout of astronomical studies are available. Star-forming regions distinguish themselves from other regions in the Galaxy. Many different physical processes are displayed with high levels of variability, a large number of outflow sources, interactions with the circumstellar medium and emissions throughout the entire electromagnetic spectrum. None of the other stages of stellar evolution appear so evidently active in extended, but limited, regions in the sky. Clearly, supernova remnants or planetary nebulae do the same, but they always represent single isolated events.
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Schulz, N.S. (2012). Star-Forming Regions. In: The Formation and Early Evolution of Stars. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-23926-7_11
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