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Table A.3

As in Table A.1, but simulated lenticular remnants resulting from numerical experiments of (giant S0)-(dwarf E0) galaxy mergers with different orbital parameters.

Galaxy θ r e n h q b q d | δ |
[°] [arcsec] [arcsec] [°]
(1) (2) (3) (4) (5) (6) (7) (8)

gS0dE0o98 0 7.8 1.1 21.5 0.49 0.90 9
180 7.9 1.1 21.6 0.49 0.91 13
30 7.4 1.1 21.7 0.52 0.82 30
45 6.8 1.2 21.9 0.54 0.70 26
60 6.4 1.2 22.4 0.54 0.53 19

gS0dE0o99 0 7.8 1.1 20.8 0.49 0.99 16
180 7.8 1.1 20.7 0.49 0.97 16
30 6.7 1.1 18.5 0.56 0.91 7
45 5.9 1.2 18.5 0.66 0.89 54
60 4.9 1.2 18.7 0.76 0.66 40

gS0dE0o100 0 8.0 1.1 21.2 0.48 0.85 1
180 8.0 1.1 21.1 0.47 0.87 1
30 7.3 1.2 20.9 0.53 0.87 38
45 6.6 1.2 22.1 0.59 0.74 44
60 5.8 1.2 22.9 0.65 0.56 31

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