Table 1.
Main photometric and kinematic properties of the sample galaxies.
Object | Re,r | Mr | (g-r) | log(M*/M⊙) | Rtr, 1 | Rtr, 2 | Rmax/Re | Fornax substructure | |
---|---|---|---|---|---|---|---|---|---|
[kpc] | [mag] | [mag] | [kpc] | [kpc] | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
FCC 083 | 3.30 ± 0.03 | −20.56 ± 0.08 | 0.69 ± 0.02 | 10.30 ± 0.05 | 5.58 ± 0.06 | ... | 2.0 | infalling | |
FCC 119 | 1.33 ± 0.02 | −17.24 ± 0.10 | 0.69 ± 0.03 | 9.15 ± 0.01 | 0.26 ± 0.05 | ... | 1.1 | infalling | |
FCC 143 | 1.029 ± 0.005 | −18.77 ± 0.12 | 0.07 ± 0.05 | 9.45 ± 0.01 | 0.561 ± 0.002 | 6.175 ± 0.007 | 2.4 | NS clump | |
FCC 147 | 2.36 ± 0.02 | −20.96 ± 0.08 | 0.64 ± 0.02 | 10.38 ± 0.03 | 0.38 ± 0.01 | ... | 2.6 | NS clump | |
FCC 148 | 2.73 ± 0.02 | −19.79 ± 0.09 | 0.63 ± 0.02 | 9.76 ± 0.04 | 0.47 ± 0.02 | 11.00 ± 0.07 | 2.1 | Infalling | |
FCC 153 | 2.00 ± 0.06 | −19.89 ± 0.12 | 0.24 ± 0.07 | 9.88 ± 0.01 | 4.29 ± 0.06 | ... | 3.2 | Infalling | |
FCC 161 | 2.76 ± 0.02 | −21.02 ± 0.05 | 0.71 ± 0.02 | 10.42 ± 0.03 | 0.27 ± 0.05 | 13.89 ± 0.12 | 2.0 | NS clump | |
FCC 167 | 5.80 ± 0.05 | −22.36 ± 0.09 | 0.59 ± 0.03 | 10.99 ± 0.05 | 4.32 ± 0.06 | 12.33 ± 0.12 | 1.9 | NS clump | |
FCC 170 | 1.69 ± 0.01 | −20.71 ± 0.09 | 0.65 ± 0.02 | 10.35 ± 0.02 | 0.86 ± 0.01 | ... | 4.3 | NS clump | |
FCC 177 | 3.48 ± 0.02 | −19.71 ± 0.07 | 0.72 ± 0.02 | 9.93 ± 0.02 | 0.211 ± 0.001 | ... | 1.6 | Infalling | |
FCC 182 | 0.941 ± 0.005 | −17.88 ± 0.10 | 0.66 ± 0.02 | 9.18 ± 0.02 | 0.47 ± 0.02 | ... | 2.2 | NS clump | |
FCC 184 | 3.223 ± 0.001 | −21.43 ± 0.13 | 0.76 ± 0.05 | 10.67 ± 0.01 | 0.926 ± 0.008 | 17.40 ± 0.33 | 2.5 | NS clump | |
FCC 190 | 1.805 ± 0.008 | −19.28 ± 0.08 | 0.66 ± 0.02 | 9.73 ± 0.03 | 0.472 ± 0.006 | 2.36 ± 0.02 | 2.1 | NS clump | |
FCC 193 | 2.90 ± 0.03 | −20.93 ± 0.09 | 0.73 ± 0.03 | 10.52 ± 0.04 | 2.82 ± 0.04 | 20.35 ± 0.33 | 2.0 | NS clump | |
FCC 219 | 15.77 ± 0.20 | −22.95 ± 0.11 | 0.71 ± 0.12 | 11.10 ± 0.01 | 3.79 ± 0.06 | ... | 0.5 | Core | |
FCC 249 | 2.19 ± 0.01 | −19.13 ± 0.12 | 0.85 ± 0.05 | 10.11 ± 0.01 | 0.32 ± 0.08 | 11.17 ± 0.12 | 3.0 | Infalling | |
FCC 255 | 2.32 ± 0.02 | −19.76 ± 0.09 | 0.84 ± 0.05 | 10.30 ± 0.01 | 4.75 ± 0.08 | ... | 2.8 | infalling | |
FCC 276 | 4.245 ± 0.007 | −21.31 ± 0.09 | 0.30 ± 0.08 | 10.26 ± 0.03 | 0.46 ± 0.04 | 12.54 ± 0.11 | 1.7 | NS clump | |
FCC 277 | 1.282 ± 0.004 | −19.24 ± 0.09 | 0.40 ± 0.03 | 9.53 ± 0.01 | 1.04 ± 0.03 | ... | 2.6 | Infalling | |
FCC 301 | 1.12 ± 0.03 | −18.82 ± 0.09 | 0.34 ± 0.06 | 9.30 ± 0.05 | 1.80 ± 0.09 | ... | 2.3 | Infalling | |
FCC 310 | 3.432 ± 0.002 | −19.70 ± 0.10 | 0.37 ± 0.09 | 9.73 ± 0.02 | 7.99 ± 0.12 | ... | 1.0 | Infalling |
Notes. (1) Galaxy name from Ferguson (1989). (2)–(5) r-band effective radius and absolute magnitude, (g − r), colour, and total stellar mass from Iodice et al. (2019b). (6) and (7) Transition radii from Spavone et al. (2020) for all the galaxies, except for FCC 119, FCC 249, and FCC 255, for which we performed the multi-component photometric fit. (8) Ratio between the maximum radial extension of the MUSE data along the galaxy major axis and r-band effective radius. (9) Galaxy sub-structure according to the phase-space analysis from Iodice et al. (2019a).
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