Astrophysics II
Radiative cooling refers to the process by which an object loses heat by emitting radiation in the form of electromagnetic waves. This phenomenon is significant in astrophysics as it impacts the temperature and thermal evolution of various astronomical entities, particularly within the interstellar medium and the intracluster medium. As gas clouds or hot plasmas cool down through radiation, they play a crucial role in the formation of stars and galaxies, and influence the overall dynamics of clusters in the universe.
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