Table A.1
Structural parameters of the simulated lenticular remnants resulting from numerical experiments of giant-giant galaxy mergers.
| Galaxy | θ | re | n | h | q b | q d | | δ | |
| [°] | [arcsec] | [arcsec] | [°] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||
| gE0gSbo5 | 0 | 0.8 | 3.8 | 9.0 | 0.95 | 0.98 | 90 |
| 180 | 0.8 | 3.8 | 9.0 | 1.00 | 0.98 | 32 | |
| 30 | 0.9 | 4.9 | 9.1 | 1.00 | 0.97 | 19 | |
| 45 | 0.9 | 3.9 | 9.4 | 0.86 | 0.78∗ | 4 | |
| 60 | 1.0 | 4.1 | 9.7 | 0.78 | 0.67∗ | 1 | |
|
|
|||||||
| gE0gSdo5 | 0 | 1.0 | 1.1 | 8.7 | 0.80 | 0.99 | 6 |
| 180 | 1.0 | 1.1 | 8.7 | 0.80 | 0.99 | 6 | |
| 30 | 0.9 | 1.2 | 8.7 | 0.90 | 0.90∗ | 23 | |
| 45 | 0.9 | 1.3 | 8.9 | 0.81 | 0.83∗ | 18 | |
| 60 | 0.8 | 1.5 | 9.1 | 0.64 | 0.70∗ | 7 | |
|
|
|||||||
| gSbgSbo9 | 0 | 1.3 | 3.5 | 10.9 | 0.72 | 0.97 | 90 |
| 180 | 1.3 | 3.5 | 10.9 | 0.72 | 0.97 | 90 | |
| 30 | 1.2 | 3.8 | 11.0 | 0.78 | 0.87 | 63 | |
| 45 | 1.1 | 4.2 | 11.3 | 0.81 | 0.74 | 42 | |
| 60 | 1.1 | 4.9 | 11.6 | 0.73 | 0.57 | 18 | |
|
|
|||||||
| gSbgSdo5 | 0 | 2.3 | 3.6 | 18.0 | 0.83 | 0.99 | 58 |
| 180 | 2.4 | 4.0 | 18.1 | 0.84 | 0.99 | 59 | |
| 30 | 2.3 | 3.8 | 18.0 | 0.82 | 0.92 | 29∗ | |
| 45 | 2.2 | 3.6 | 17.4 | 0.75 | 0.82 | 21∗ | |
| 60 | 2.1 | 3.5 | 17.4 | 0.64 | 0.67 | 12∗ | |
Notes. (1) Identifier of the simulated lenticular remnant. (2) Galaxy inclination. (3) Effective radius of the bulge. (4) Sérsic index of the bulge. (5) Scale length of the disk. (6), (7) Apparent axial ratio of the bulge and disk, respectively. (8) Difference of the position angles of bulge and disk. Nominal values are marked with ∗.
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