Using new UV magnitudes for a sample of early-type galaxies (ETGs) with published stellar mass-to-light ratios, Υ*, we find a correlation between UV color and Υ* that is tighter than those previously identified between Υ* and either the central stellar velocity dispersion, metallicity, or alpha enhancement. The sense of the correlation is that galaxies with larger Υ* are bluer in the UV. We conjecture that differences in the lower mass end of the stellar initial mass function (IMF) are related to the nature of the extreme horizontal branch populations that are generally responsible for the UV flux in ETGs. If so, then UV color can be used to identify ETGs with particular IMF properties and to estimate Υ*.
- galaxies: elliptical and lenticular cD
- galaxies: evolution
- galaxies: stellar content
- stars: luminosity function mass function
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science