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Dynamical versus stellar masses of ultracompact dwarf galaxies in the Fornax cluster star

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Academic year: 2020

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Figure

Figure 1. A fragment of the science frame before (top) and after (bottom) diffuse light subtraction
Table 1. Coordinates of 6 UCDs excluded from the final sample of Mieske et al. (2008).
Figure 3. FLAMES/Giraffe HR9 spectra, their best-fitting templates (Kroupa IMF), fitting residuals and confidence levels of the age and metallicity determinations (inner panels)
Figure 4. Continuation of Fig 3.
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