Table 2
Input parameters for the LB simulations.
| texp (Myr) |
X (pc) |
Y (pc) |
Z (pc) |
D (pc) |
U (km s−1) |
V (km s−1) |
W (km s−1) |
Mini (M⊕) |
Mej (10−4 M⊙) |
Mrem (M⊙) |
Pop.(a) | ||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 26Al | 53Mn | 60Fe | |||||||||||
| −10.16 | 45.5 | 27.3 | 18.6 | 236.4 | 6.3 | −8.7 | 6.6 | 21.69 | 1.00 | 0.88 | 2.84 | 2.90 | c |
| −9.68 | 64.5 | 21.9 | 9.8 | 238.7 | 3.1 | −7.4 | 6.5 | 20.42 | 0.87 | 0.83 | 3.86 | 2.92 | c |
| −8.90 | 31.2 | −24.7 | 16.1 | 178.9 | −0.7 | −9.0 | 0.4 | 19.32 | 0.75 | 3.50 | 3.72 | 2.86 | c |
| −8.00 | 30.3 | −26.5 | 17.8 | 161.2 | −0.5 | −9.3 | 0.9 | 18.34 | 0.64 | 7.35 | 3.04 | 2.75 | c |
| −7.20 | 31.1 | −35.3 | 15.6 | 143.7 | −1.0 | −9.0 | 0.5 | 17.47 | 0.55 | 10.78 | 2.43 | 2.65 | c |
| −7.07 | 113.1 | −15.6 | 7.3 | 220.9 | 4.8 | −9.0 | 4.5 | 17.32 | 0.54 | 11.35 | 2.33 | 2.64 | v |
| −6.48 | 33.5 | −40.5 | 28.7 | 136.4 | 0.7 | −8.8 | 3.4 | 16.69 | 0.47 | 13.86 | 1.88 | 2.57 | c |
| −5.84 | 31.2 | −50.8 | 32.0 | 123.0 | 1.4 | −9.3 | 2.5 | 15.98 | 0.39 | 16.63 | 1.39 | 2.49 | c |
| −5.25 | 33.5 | −57.8 | 34.4 | 115.8 | 0.9 | −9.9 | 3.2 | 15.34 | 0.32 | 19.16 | 0.94 | 2.42 | c |
| −4.48 | 37.5 | −57.6 | 19.4 | 101.2 | 0.2 | −9.4 | 0.3 | 14.76 | 0.28 | 18.12 | 0.71 | 2.37 | c |
| −3.47 | 40.9 | −65.9 | 19.5 | 92.2 | 0.5 | −8.7 | 0.4 | 14.22 | 0.25 | 12.83 | 0.74 | 2.33 | c |
| −2.54 | 33.5 | −74.3 | 28.2 | 83.1 | 1.5 | −9.3 | 0.9 | 13.73 | 0.23 | 7.95 | 0.77 | 2.30 | c |
| −1.68 | 99.3 | −18.0 | 55.6 | 128.5 | 5.6 | −6.4 | 4.5 | 13.28 | 0.21 | 3.45 | 0.79 | 2.27 | c |
| −0.88 | 47.7 | −87.1 | 19.4 | 96.0 | 1.6 | −8.6 | −0.2 | 12.85 | 0.20 | 0.72 | 0.81 | 2.25 | c |
Notes. The table lists the explosion times of the past SN events in the Sco-Cen complex (texp), the Cartesian coordinates of their explosion centres with respect to the LSR (X, Y, Z), the distances of the explosion sites to the actual position of the Sun (D), the final peculiar velocity components of the SN progenitor stars (U, V, W), their initial masses (Mini), the 26Al, 53Mn, and 60Fe masses ejected during the explosions (Mej), the masses of the stellar remnants (Mrem), and the stellar populations in which the explosions took place.(a) c = UCL/LCC; v = V1062 Sco.
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