Table 1
Parameters of the minor and intermediate merger experiments.
| Model code | Msat/Mprim | Rper/hD,prim | θ | (B/D)prim | α TF |
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| (a) M6 Ps Db | 1:6 (M6) | 0.73 (Ps) | 30 (D) | 0.5 (b) | 3.5 |
| (a2) M6 Ps Db TF3 | 1:6 (M6) | 0.73 (Ps) | 30 (D) | 0.5 (b) | 3.0 |
| (a3) M6 Ps Db TF4 | 1:6 (M6) | 0.73 (Ps) | 30 (D) | 0.5 (b) | 4.0 |
| (b) M6 Ps Rb | 1:6 (M6) | 0.73 (Ps) | 150 (R) | 0.5 (b) | 3.5 |
| (c) M6 Pl Db | 1:6 (M6) | 8.25 (Pl) | 30 (D) | 0.5 (b) | 3.5 |
| (d) M6 Pl Rb | 1:6 (M6) | 8.25 (Pl) | 150 (R) | 0.5 (b) | 3.5 |
| (e) M6 Ps Ds | 1:6 (M6) | 0.87 (Ps) | 30 (D) | 0.08 (s) | 3.5 |
| (f) M6 Ps Rs | 1:6 (M6) | 0.87 (Ps) | 150 (R) | 0.08 (s) | 3.5 |
|
|
|||||
| (g) M9 Ps Db | 1:9 (M9) | 0.79 (Ps) | 30 (D) | 0.5 (b) | 3.5 |
| (g2) M9 Ps Db TF3 | 1:9 (M9) | 0.79 (Ps) | 30 (D) | 0.5 (b) | 3.0 |
| (g3) M9 Ps Db TF4 | 1:9 (M9) | 0.79 (Ps) | 30 (D) | 0.5 (b) | 4.0 |
| (h) M9 Ps Rb | 1:9 (M9) | 0.79 (Ps) | 150 (R) | 0.5 (b) | 3.5 |
|
|
|||||
| (i) M18 Ps Db | 1:18 (M18) | 0.86 (Ps) | 30 (D) | 0.5 (b) | 3.5 |
| (j) M18 Ps Rb | 1:18 (M18) | 0.86 (Ps) | 150 (R) | 0.5 (b) | 3.5 |
| (k) M18 Pl Db | 1:18 (M18) | 8.19 (Pl) | 30 (D) | 0.5 (b) | 3.5 |
| (l) M18 Pl Rb | 1:18 (M18) | 8.19 (Pl) | 150 (R) | 0.5 (b) | 3.5 |
|
|
|||||
Notes. Columns: (1) Model code: MmP[l/s][D/R][b/s][TF3/4], see the text. (2) Luminous mass ratio between the satellite and the primary S0 galaxy. (3) Orbital first pericentre distance in units of the primary disc scale-length. (4) Initial angle between the angular momenta of the orbit and the primary disc. (5) Bulge-to-disc ratio of the original primary S0: B/D = 0.5 (S0b) or B/D = 0.08 (S0c). (6) Value of α TF assumed for the scaling of the satellite to the primary S0. More details of the models in EM06 and EM11.
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