Table 3.
Physical parameters of the thin and thick discs of each galaxy in our sample.
Phys. param. | NGC | 0429 | NGC | 01040 | UGC | 00931 | UGC | 01839 | UGC | 1032 |
---|---|---|---|---|---|---|---|---|---|---|
zt [kpc] | 1.14 | 1.38 | 0.31 | 0.36 | 0.31 | 0.35 | 0.31 | 0.28 | 1.74 | 1.8 |
zT [kpc] | 5.15 | 5.75 | 1.13 | 0.91 | 0.61 | 0.53 | 0.6 | 0.47 | 8.82 | 8.81 |
zT/zt | 4.51 | 4.17 | 3.64 | 2.53 | 1.96 | 1.51 | 1.93 | 1.68 | 5.07 | 4.89 |
ρ0T/ρ0t | 0.09 | 0.04 | 0.16 | 0.09 | 0.24 | 0.33 | 0.29 | 1.31 | 0.11 | 0.13 |
ΣT/Σt | 0.34 | 0.15 | 0.5 | 0.22 | 0.45 | 0.46 | 0.51 | 2.19 | 0.42 | 0.49 |
ΥT/Υt | – | 0.99 | – | 1.07 | – | 1.97 | – | 1.46 | – | 0.56 |
Notes. Weighted mean values of the physical parameters of thin and thick discs of each galaxy for the observed data (left values of each column) and for the PSF-deconvolved models (right values of each column). These results are obtained from the vertical fits of the light distribution determined by solving a system of equations that describe two gravitationally coupled vertically isothermal discs (thin and thick discs). The mass-to-light ratios between the thin and thick discs ((M/L)T/(M/L)t = ΥT/Υt) is only obtained for the PSF-deconvolved models. For more details about the parameters, see Sect. 5.2.2.
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