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Mass-to-light ratio gradients in early-type galaxy haloes

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Academic year: 2021

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Figure

Figure 1. Profiles of enclosed mass with radius. Each panel shows a galaxy with parameters indicated
Figure 3. Predictions for the M / L gradient versus total stellar mass from CDM, for different values of the star formation efficiency SF
Table 1. Catalogue of early-type galaxies with halo mass measurements.
Figure 4. Estimates of stellar M / L from stellar population synthesis mod- mod-elling ( ϒ SSP ) compared to dynamical modelling ( ϒ in ), in units of ϒ B ,
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