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- W3100272244 abstract "Using 3.6 and 4.5 μm images of 73 late-type, edge-on galaxies from the S4G survey, we compare the richness of the globular cluster populations of these galaxies to those of early-type galaxies that we measured previously. In general, the galaxies presented here fill in the distribution for galaxies with lower stellar mass, M*, specifically , overlap the results for early-type galaxies of similar masses, and, by doing so, strengthen the case for a dependence of the number of globular clusters per 109M⊙ of galaxy stellar mass, TN, on M*. For we find the relationship can be satisfactorily described as when M* is expressed in solar masses. The functional form of the relationship is only weakly constrained, and extrapolation outside this range is not advised. Our late-type galaxies, in contrast to our early types, do not show the tendency for low-mass galaxies to split into two TN families. Using these results and a galaxy stellar mass function from the literature, we calculate that, in a volume-limited, local universe sample, clusters are most likely to be found around fairly massive galaxies (M* ∼ 1010.8M⊙) and present a fitting function for the volume number density of clusters as a function of parent-galaxy stellar mass. We find no correlation between TN and large-scale environment, but we do find a tendency for galaxies of fixed M* to have larger TN if they have converted a larger proportion of their baryons into stars." @default.
- W3100272244 created "2020-11-23" @default.
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- W3100272244 date "2016-02-10" @default.
- W3100272244 modified "2023-10-09" @default.
- W3100272244 title "GLOBULAR CLUSTER POPULATIONS: RESULTS INCLUDING S4G LATE-TYPE GALAXIES" @default.
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- W3100272244 doi "https://doi.org/10.3847/0004-637x/818/1/99" @default.
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