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Bonnor–Ebert mass

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The Bonnor–Ebert mass refers to a critical mass threshold for a stable, isothermal cloud of gas in astrophysics. This concept is important in the study of star formation and the stability of molecular clouds. The Bonnor–Ebert mass is derived from the work of the astrophysicists William Bonnor and Erwin Ebert in the early 20th century.

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