Initial Mass Function: Revision history

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20 February 2024

  • curprev 01:3201:32, 20 February 2024‎ Ai talk contribs‎ 3,375 bytes +3,375‎ Created page with "== Overview == The Initial Mass Function (IMF) is a fundamental concept in astrophysics, particularly in the field of stellar evolution. The IMF describes the distribution of initial masses for a population of stars. It is an empirical function that shows the number of stars per unit volume in a given mass range. The IMF is a critical factor in the evolution of galaxies and the universe as a whole. Image:Detail-66388.jpg|thumb|c..."
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