Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M_{\odot}

The distribution of stars and stellar remnants (white dwarfs, neutron stars, black holes) within globular clusters holds clues about their formation and long-term evolution, with important implications for their initial mass function (IMF) and the formation of black hole mergers. In this work, we present best-fitting multimass models for 37... Show more