CORDIS Project
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The Stellar Populations and Dynamical project investigates variations in the initial mass function of stars, which influences galaxy formation and evolution. By combining stellar population studies with dynamical techniques, it aims to enhance our understanding of star formation across different galaxies.
The number distribution of stars by mass in a stellar system, at birth, is given by the initial mass function (IMF).
The IMF not only regulates the chemical enrichment of a galaxy, but it also determines its spectrum and the mass scale.
Moreover, it is the bridge between the physics and properties of individual stars and the light that we observe from distant galaxies.
Therefore, the IMF constitutes a fundamental piece in modern Astrophysics.
Since the pioneers works suggested an invariant IMF i…
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
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LOS ANGELES UCLA SANTA BARBARA UCSB DAVIS UCD RIVERSIDE UCR SAN DIEGO UCSD SANTA CRUZ UCSC IRVIN
United States, Berkeley
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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