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Table 2

Structural and kinematic properties of the progenitors and the remnants when considered as single-component systems.

Model Reff,glx/reff,bulge ϵe (V/σ)e λe (from Eq. (1)) λe (from Eq. (4)) δglx (from Eq. (5))
(1) (2) (3) (4) (5) (6) (7)
Original S0b, B/D = 0.5 4.59 0.875 ± 0.017 0.466 ± 0.002 0.468 ± 0.002 0.456 ± 0.002 0.3959 ± 0.008
Original S0c, B/D = 0.08 8.94 0.869 ± 0.003 1.469 ± 0.023 0.819 ± 0.014 0.850 ± 0.018 0.9126 ± 0.0008
(a)    M6 Ps Db 5.19 0.683 ± 0.002 0.439 ± 0.001 0.413 ± 0.001 0.435 ± 0.001 0.37 ± 0.04
(a2) M6 Ps Db TF3 5.06 0.694 ± 0.004 0.299 ± 0.015 0.303 ± 0.019 0.312 ± 0.017 0.36 ± 0.08
(a3) M6 Ps Db TF4 4.83 0.651 ± 0.002 0.284 ± 0.007 0.294 ± 0.010 0.298 ± 0.008 0.34 ± 0.06
(b)    M6 Ps Rb 4.93 0.681 ± 0.008 0.224 ± 0.013 0.271 ± 0.018 0.239 ± 0.014 0.37 ± 0.08
(c)    M6 Pl Db 4.57 0.638 ± 0.009 0.337 ± 0.020 0.331 ± 0.025 0.348 ± 0.022 0.471 ± 0.010
(d)    M6 Pl Rb 4.71 0.719 ± 0.004 0.231 ± 0.001 0.234 ± 0.001 0.246 ± 0.001 0.45 ± 0.16
(e)    M6 Ps Ds 8.52 0.755 ± 0.011 0.735 ± 0.011 0.632 ± 0.012 0.629 ± 0.010 0.735 ± 0.002
(f)    M6 Ps Rs 10.36 0.778 ± 0.004 0.494 ± 0.016 0.463 ± 0.019 0.478 ± 0.017 0.701 ± 0.005
(g)    M9 Ps Db 5.09 0.697 ± 0.008 0.298± 0.023 0.318 ± 0.030 0.312 ± 0.025 0.36 ± 0.05
(g2) M9 Ps Db TF3 5.26 0.727 ± 0.006 0.292 ± 0.022 0.313 ± 0.028 0.306 ± 0.024 0.36 ± 0.01
(g3) M9 Ps Db TF4 4.61 0.671 ± 0.002 0.285 ± 0.014 0.307 ± 0.019 0.299 ± 0.016 0.34 ± 0.08
(h)    M9 Ps Rb 5.35 0.713 ± 0.005 0.222 ±0.005 0.235 ± 0.006 0.237 ± 0.005 0.393 ± 0.002
(i)    M18 Ps Db 5.05 0.769 ± 0.004 0.265 ± 0.009 0.280 ± 0.012 0.280 ± 0.010 0.365 ± 0.023
(j)    M18 Ps Rb 5.27 0.802 ± 0.005 0.328 ± 0.009 0.357 ± 0.012 0.339 ± 0.010 0.38 ± 0.07
(k)   M18 Pl Db 4.77 0.704 ± 0.006 0.311 ± 0.017 0.346 ± 0.023 0.324 ± 0.019 0.442 ± 0.003
(l)    M18 Pl Rb 5.10 0.743 ± 0.004 0.381 ± 0.020 0.408 ± 0.027 0.387 ± 0.022 0.454 ± 0.010

Notes. Columns: (1) Model code. (2) Ratio between the half-mass radius of each galaxy and the effective radius of its bulge. The bulge effective radii are available in Table 2 of Eliche-Moral et al. (2013). (3, 4) Ellipticity within r = Reff,glx and the (V/σ)e value computed from N-body data following the procedure by E11, for edge-on views of the galaxies. (5) The λe kinematic parameter defined by Emsellem et al. (2007) directly measured from N-body data (using the definition in Eq. (1)), for an edge-on view of each galaxy. (6) The λe kinematic parameter derived using Eq. (4), using the measured values of (V/σ)e in Col. 4, assuming κ = 1.1 (see E11). (7) Anisotropy of velocities in the models, computed directly from the data using Eq. (5).

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