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Table 4.

Results of the fit of jt versus M* with the power law in Eq. (10).

Group of data A log10j0 σ
[dex]
Ellipticals
jt, light − M* 0.74 ± 0.22 2.52 ± 0.09 0.22
jt, mass − M* 0.76 ± 0.23 2.45 ± 0.10 0.24
jt, mass + IMF − M*, var IMF 0.73 ± 0.27 2.28 ± 0.13 0.30

Lenticulars
jt, light − M* 0.54 ± 0.16 2.85 ± 0.08 0.19
jt, mass − M* 0.55 ± 0.17 2.78 ± 0.08 0.20
jt, mass + IMF − M*, var IMF 0.45 ± 0.16 2.68 ± 0.08 0.21

Slow rotators
jt, light − M* 0.49 ± 0.30 2.67 ± 0.14 0.17
jt, mass − M* 0.50 ± 0.33 2.60 ± 0.16 0.18
jt, mass + IMF − M*, var IMF 0.47 ± 0.34 2.48 ± 0.18 0.19

Fast rotators
jt, light − M* 0.57 ± 0.19 2.69 ± 0.12 0.29
jt, mass − M* 0.59 ± 0.21 2.62 ± 0.10 0.30
jt, mass + IMF − M*, var IMF 0.47 ± 0.22 2.5 ± 0.11 0.38

Notes. The rightmost column lists the unweighted orthogonal scatter σ of the data points around the fitted relations. The errors on the parameters are the sum in quadrature of the error on the fit to the unweighted data-points, and the root-mean-square sigma of the distribution of parameters from fitting Monte Carlo simulations of the jt values sampled from their errors. See Sect. 8.2.

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