Stellar Initial Mass Function Varies with Metallicity and Age of Stars
In the vast and diverse Universe, the initial mass distribution at the birth of a new population of stars determines the fate of galaxies. This relationship is described by the Initial Mass Function (IMF). For more than half a century, astronomers have assumed that the IMF is a universal relationship, i.e., it is uniform throughout the Universe.
In the vast and diverse Universe, the initial mass distribution at the birth of a new population of stars determines the fate of galaxies. This relationship is described by the Initial Mass Function (IMF). For more than half a century, astronomers have assumed that the IMF is a universal relationship, i.e., it is uniform throughout the Universe.However, in recent years, some indications suggest...
Jun 13, 2025