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Table 1

Intrinsic shape of the bulges of the simulated lenticular remnants seen at different inclinations.

Galaxy B/A C/A
() (180°) (30°) (45°) (60°) (30°) (45°) (60°)
(1) (2) (3) (4) (5) (6) (7) (8) (9)

gE0gSbo5 1.00 1.00 1.00 1.00 1.00 0.99 0.59 0.59
gE0gSdo5 0.79 0.79 0.91 0.89 0.86 0.46 0.26 0.26
gS0dE0o98 0.46 0.49 0.49 0.64 0.56 0.51 0.21 0.36
gS0dE0o99 0.46 0.46 0.54 0.59 0.69 0.64 0.64 0.64
gS0dE0o100 0.46 0.46 0.49 0.54 0.56 0.59 0.14 0.39
gS0dS0o99 0.59 0.59 0.56 0.61 0.76 0.64 0.41 0.21
gS0dSao103 0.51 0.51 0.51 0.56 0.56 0.96 0.21 0.34
gS0dSbo106 0.44 0.44 0.41 0.46 0.61 0.69 0.39 0.29
gS0dSdo100 0.51 0.51 0.49 0.51 0.74 0.54 0.41 0.24
gSbgSbo9 0.71 0.71 0.76 0.76 0.76 1.06 0.74 0.54
gSbgSdo5 0.81 0.84 0.84 0.81 0.84 0.36 0.26 0.21

Notes. (1) Identifier in the GalMer database of the merger experiment resulting in a lenticular remnant, which we adopted as the name of the simulated galaxy. (2)–(6) Intrinsic axial ratio B/A of the bulge obtained from the mock images of the simulated lenticular remnants seen at an inclination θ = 0°, 180°, 30°, 45°, and 60°, respectively. (7)–(9) Intrinsic axial ratio C/A of the bulge obtained from the mock images of the simulated lenticular remnants seen at an inclination θ = 30°, 45°, and 60°, respectively.

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