Converting Hα Luminosities into Star Formation Rates
Star formation rates (SFRs) of galaxies are commonly calculated by converting the measured Hα luminosities (LHα) into current SFRs. This conversion is based on a constant initial mass function (IMF) independent of the total SFR. As was recently recognized, the maximum stellar mass in a star cluster is limited by the embedded total cluster mass and
Pflamm-Altenburg, Jan et al.
Advertised on:
12
2007