The Variation of Integrated Star Initial Mass Functions among Galaxies
The integrated galaxial initial mass function (IGIMF) is the relevant distribution function containing the information on the distribution of stellar remnants, the number of supernovae, and the chemical enrichment history of a galaxy. Since most stars form in embedded star clusters with different masses, the IGIMF becomes an integral of the assumed
Weidner, C. et al.
Fecha de publicación:
6
2005