Table 4.
Median difference of the global stellar population properties and HLR between galaxies in the two samples (voids – filaments and walls), for each morphological type.
| HType | Δlog M⋆ [M⊙] | Δlog Σ⋆ [M⊙ pc−2] | Δ ⟨log t⟩L [yr] | Δlog SFR [M⊙ yr−1] | Δlog sSFR [Gyr−1] | Δlog HLR [kpc] |
|---|---|---|---|---|---|---|
| E | −0.06 ± 0.18 | −0.24 ± 0.20 | −0.07 ± 0.29 | −0.15 ± 1.20 (3) | 0.54 ± 1.15 | 0.14 ± 0.13 |
| S0 | −0.00 ± 0.13 | −0.11 ± 0.25 | 0.03 ± 0.31 | 1.51 ± 0.03 (2) | 1.52 ± 0.02 | 0.06 ± 0.16 |
| Sa | −0.01 ± 0.09 | −0.19 ± 0.20 | −0.26 ± 0.36 | 0.40 ± 0.44 (10) | 0.44 ± 0.44 | 0.08 ± 0.21 |
| Sb | −0.00 ± 0.14 | −0.17 ± 0.26 | −0.09 ± 0.48 | 0.14 ± 0.81 (23) | 0.14 ± 0.82 | −0.03 ± 0.18 |
| Sc | 0.00 ± 0.13 | −0.18 ± 0.25 | −0.33 ± 0.41 | 0.13 ± 0.60 (50) | 0.13 ± 0.58 | 0.02 ± 0.21 |
| Sd | −0.09 | −0.37 | −0.33 | 0.15 (1) | 0.24 | 0.15 |
Notes. The uncertainty is given by the standard deviation of the distribution. The last row belongs to the difference in the values of the single Sd galaxy in each sample. The values between brackets in the Δlog SFR column refer to the number of pairs taken into account to calculate the difference in log SFR and log sSFR (those in which none of the values were masked).
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