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Table A.2

Mean orbital characteristics with the dispersion (characterized by standard deviation) of the predicted annual meteor showers associated with the parent body considered.

Filament q a e ω Ω i Ns
tev = 1 kyr, β = 0.005
01aI 0.335 ± 0.015 2.3 ± 0.0 0.856 ± 0.005 301.4 ± 20.2 223.9 ± 20.0 3.1 ± 0.7 713
tev = 1 kyr, β = 0.007
xI 0.334 ± 0.011 2.3 ± 0.0 0.854 ± 0.004 298.3 ± 18.7 227.0 ± 18.4 3.1 ± 0.6 230
xII 0.323 ± 0.019 2.300 ± 0.1 0.857 ± 0.007 224.7 ± 15.6 299.6 ± 15.3 3.8 ± 0.8 1360
tev = 1 kyr, β = 0.009
01cII 0.362 ± 0.008 2.4 ± 0.0 0.848 ± 0.003 291.4 ± 19.5 236.5 ± 19.6 2.9 ± 0.6 30
01cIII 0.358 ± 0.002 2.300 ± 0.1 0.842 ± 0.004 241.2 ± 9.7 286.4 ± 9.5 3.1 ± 0.4 143
02cI 0.511 ± 0.015 2.500 ± 0.0 0.798 ± 0.005 297.5 ± 13.6 230.7 ± 13.4 2.9 ± 0.4 191
02cII 0.512 ± 0.007 2.500 ± 0.0 0.798 ± 0.002 233.0 ± 11.3 294.6 ± 11.3 3.2 ± 0.3 155
tev = 1 kyr, β = 0.011
01dI 0.268 ± 0.052 2.2 ± 0.1 0.878 ± 0.017 306.8 ± 20.7 217.8 ± 20.2 3.3 ± 0.9 1291
01dII 0.272 ± 0.066 2.200 ± 0.1 0.877 ± 0.022 226.9 ± 22.3 297.4 ± 22.1 3.9 ± 1.2 577
tev = 2 kyr, β = 0.00001
01eI 0.331 ± 0.015 2.3 ± 0.0 0.854 ± 0.006 223.3 ± 12.1 299.6 ± 12.2 4.2 ± 0.7 750
tev = 2 kyr, β = 0.0001
01fI 0.327 ± 0.015 2.3 ± 0.0 0.855 ± 0.006 221.4 ± 10.9 301.5 ± 10.9 4.3 ± 0.7 852
tev = 2 kyr, β = 0.001
01gI 0.307 ± 0.011 2.2 ± 0.0 0.863 ± 0.004 215.0 ± 4.4 307.9 ± 4.2 4.8 ± 0.4 908
tev = 2 kyr, β = 0.003
01hI 0.317 ± 0.024 2.2 ± 0.0 0.859 ± 0.009 286.7 ± 14.7 237.6 ± 14.6 3.3 ± 0.4 297
01hIII 0.317 ± 0.041 2.2 ± 0.0 0.858 ± 0.015 234.2 ± 17.2 289.5 ± 16.8 4.1 ± 0.9 1343
tev = 2 kyr, β = 0.005
01iI 0.303 ± 0.018 2.2 ± 0.0 0.861 ± 0.007 301.3 ± 18.1 222.8 ± 18.0 4.2 ± 0.9 1060
01iII 0.306 ± 0.033 2.2 ± 0.1 0.859 ± 0.012 231.7 ± 17.4 291.7 ± 17.2 4.5 ± 0.9 1781
tev = 2 kyr, β = 0.007
01jI 0.312 ± 0.025 2.1 ± 0.1 0.854 ± 0.009 295.5 ± 17.4 228.4 ± 17.3 4.3 ± 0.8 528
01jII 0.448 ± 0.014 2.4 ± 0.0 0.814 ± 0.005 304.7 ± 116.6 228.1 ± 16.4 3.1 ± 0.5 208
01jIII 0.330 ± 0.056 2.2 ± 0.1 0.848 ± 0.017 234.5 ± 16.5 289.9 ± 16.0 4.4 ± 1.0 1393
tev = 2 kyr, β = 0.009
03cI 0.240 ± 0.033 2.0 ± 0.1 0.880 ± 0.013 311.1 ± 16.3 210.8 ± 16.3 6.3 ± 1.2 1164
03cII 0.243 ± 0.031 2.0 ± 0.1 0.878 ± 0.012 231.8 ± 14.9 289.8 ± 14.8 6.3 ± 1.3 972
tev = 2 kyr, β = 0.011
06cI 0.250 ± 0.043 1.9 ± 0.1 0.871 ± 0.016 307.2 ± 16.0 214.7 ± 15.8 6.0 ± 1.1 1337
06cII 0.243 ± 0.030 1.9 ± 0.1 0.873 ± 0.011 231.4 ± 14.8 289.9 ± 14.7 6.5 ± 1.3 771
tev = 4 kyr, β = 0.00001
01kI 0.335 ± 0.019 2.3 ± 0.0 0.852 ± 0.008 310.4 ± 18.7 214.1 ± 18.4 3.9 ± 0.9 614
01kII 0.333 ± 0.018 2.2 ± 0.0 0.852 ± 0.008 230.2 ± 16.9 293.6 ± 16.7 3.8 ± 0.8 496
tev = 4 kyr, β = 0.0001
01lI 0.328 ± 0.020 2.3 ± 0.0 0.855 ± 0.008 310.8 ± 18.9 213.3 ± 18.6 3.9 ± 0.9 582
01lII 0.328 ± 0.020 2.2 ± 0.0 0.854 ± 0.008 231.2 ± 16.5 292.4 ± 16.4 3.7 ± 0.8 460
tev = 4 kyr, β = 0.001
01mI 0.319 ± 0.019 2.2 ± 0.0 0.856 ± 0.007 292.7 ± 16.8 231.7 ± 16.6 3.2 ± 0.5 200
01mII 0.307 ± 0.015 2.2 ± 0.0 0.860 ± 0.006 230.3 ± 16.4 292.9 ± 15.9 4.0 ± 0.8 933
tev = 4 kyr, β = 0.003
01nI 0.332 ± 0.017 2.2 ± 0.0 0.846 ± 0.006 301.1 ± 17.4 225.5 ± 16.9 3.8 ± 0.7 53
01nIII 0.374 ± 0.064 2.2 ± 0.1 0.830 ± 0.023 226.8 ± 13.6 300.1 ± 12.9 4.3 ± 0.8 415
tev = 4 kyr, β = 0.005
01oII 0.276 ± 0.017 2.0 ± 0.1 0.860 ± 0.007 223.4 ± 14.1 300.0 ± 13.8 5.2 ± 0.9 306
tev = 4 kyr, β = 0.007
04gI 0.283 ± 0.020 1.9 ± 0.1 0.849 ± 0.008 307.0 ± 17.6 218.2 ± 16.9 4.4 ± 0.8 818
04gII 0.274 ± 0.021 1.8 ± 0.1 0.851 ± 0.008 235.7 ± 20.3 287.1 ± 19.5 4.6 ± 1.1 429
tev = 4 kyr, β = 0.009
01pII 0.282 ± 0.048 1.7 ± 0.2 0.837 ± 0.014 227.0 ± 15.0 294.9 ± 14.8 5.8 ± 1.5 1150
08aI 0.196 ± 0.003 1.2 ± 0.0 0.838 ± 0.002 147.0 ± 1.4 1.8 ± 1.4 9.0 ± 0.2 53
tev = 4 kyr, β = 0.011
01qI 0.240 ± 0.030 1.4 ± 0.2 0.833 ± 0.008 310.3 ± 16.8 208.0 ± 17.1 6.1 ± 1.3 269
01qII 0.231 ± 0.032 1.4 ± 0.2 0.833 ± 0.008 227.3 ± 15.4 289.9 ± 14.8 7.1 ± 1.9 378
08bI 0.201 ± 0.004 1.0 ± 0.1 0.809 ± 0.002 144.8 ± 1.5 363.3 ± 1.5 8.4 ± 0.2 18
10aI 0.605 ± 0.047 2.1 ± 0.1 0.717 ± 0.014 277.7 ± 23.9 245.8 ± 24.7 4.6 ± 0.6 13
tev = 8 kyr, β = 0.00001
01rI 0.336 ± 0.024 2.200 ± 0.100 0.851 ± 0.010 304.3 ± 17.5 220.8 ± 17.5 3.7 ± 0.8 243
01rII 0.329 ± 0.020 2.200 ± 0.0 0.853 ± 0.009 232.5 ± 16.6 291.8 ± 16.3 3.8 ± 0.7 290
11aI 0.259 ± 0.016 2.3 ± 0.0 0.885 ± 0.007 119.2 ± 14.7 43.4 ± 14.7 6.2 ± 0.8 405
11aII 0.253 ± 0.012 2.300 ± 0.0 0.888 ± 0.005 55.5 ± 14.2 107.0 ± 14.1 6.6 ± 1.4 584
tev = 8 kyr, β = 0.0001
01sI 0.322 ± 0.021 2.2 ± 0.0 0.856 ± 0.009 305.8 ± 17.7 218.0 ± 17.7 3.9 ± 0.8 221
01sII 0.323 ± 0.021 2.2 ± 0.0 0.855 ± 0.009 232.4 ± 16.4 291.4 ± 16.5 3.9 ± 0.7 262
11bI 0.277 ± 0.014 2.3 ± 0.0 0.877 ± 0.006 118.8 ± 16.2 43.7 ± 16.2 6.2 ± 0.9 384
11bII 0.269 ± 0.013 2.3 ± 0.0 0.881 ± 0.005 55.7 ± 14.7 106.6 ± 14.6 6.6 ± 1.0 520
tev = 8 kyr, β = 0.001
05cI 0.265 ± 0.012 2.0 ± 0.0 0.865 ± 0.006 123.2 ± 14.6 27.4 ± 14.1 6.6 ± 0.9 1251
05cII 0.258 ± 0.008 1.9 ± 0.0 0.866 ± 0.003 57.2 ± 13.3 91.0 ± 12.6 6.7 ± 0.9 1158
tev = 8 kyr, β = 0.003
05dI 0.243 ± 0.023 1.7 ± 0.1 0.856 ± 0.010 127.0 ± 13.5 24.6 ± 37.9 7.4 ± 1.0 804
05dIII 0.235 ± 0.021 1.6 ± 0.1 0.858 ± 0.009 49.1 ± 11.8 96.0 ± 11.3 8.3 ± 1.2 1118
tev = 8 kyr, β = 0.005
05eI 0.267 ± 0.021 1.5 ± 0.1 0.822 ± 0.008 128.3 ± 11.4 20.4 ± 10.8 7.7 ± 0.7 80
05eIII 0.261 ± 0.023 1.5 ± 0.1 0.822 ± 0.008 47.6 ± 9.8 97.5 ± 9.3 9.1 ± 1.1 217
14aI 0.205 ± 0.014 1.0 ± 0.1 0.805 ± 0.003 326.2 ± 9.7 163.7 ± 9.0 7.7 ± 0.8 461
15aI 0.326 ± 0.018 1.8 ± 0.0 0.819 ± 0.007 305.0 ± 18.6 227.4 ± 17.8 4.1 ± 0.8 127
15aII 0.312 ± 0.020 1.8 ± 0.1 0.823 ± 0.009 235.8 ± 17.6 293.3 ± 16.7 4.3 ± 0.8 108
tev = 8 kyr, β = 0.007
05fI 0.297 ± 0.025 1.4 ± 0.1 0.790 ± 0.008 127.4 ± 12.9 24.5 ± 12.2 7.1 ± 0.6 238
05fII 0.274 ± 0.026 1.3 ± 0.1 0.788 ± 0.008 50.0 ± 10.8 96.1 ± 9.9 9.1 ± 1.2 176
14bI 0.197 ± 0.009 0.7 ± 0.1 0.733 ± 0.010 332.2 ± 5.7 154.3 ± 5.3 10.4 ± 0.7 140
18aI 0.416 ± 0.023 1.9 ± 0.1 0.786 ± 0.009 297.8 ± 16.1 248.7 ± 16.3 3.5 ± 0.5 125
tev = 16 kyr, β = 0.00001
xI 0.306 ± 0.008 2.200 ± 0.0 0.859 ± 0.004 118.4 ± 15.1 33.4 ± 14.7 5.9 ± 0.8 604
xII 0.244 ± 0.016 2.300 ± 0.0 0.892 ± 0.007 125.0 ± 15.3 42.3 ± 15.5 6.7 ± 1.1 120
xIII 0.330 ± 0.025 2.200 ± 0.000 0.853 ± 0.011 309.0 ± 16.9 217.6 ± 16.6 3.9 ± 0.8 207
xIV 0.339 ± 0.008 2.300 ± 0.000 0.852 ± 0.003 115.6 ± 14.1 62.5 ± 13.6 5.9 ± 0.7 290
xV 0.303 ± 0.005 2.200 ± 0.000 0.860 ± 0.002 59.7 ± 15.0 90.2 ± 14.6 6.1 ± 0.8 599
xV I 0.283 ± 0.017 2.200 ± 0.0 0.870 ± 0.006 71.7 ± 14.0 83.0 ± 13.1 5.6 ± 0.9 18
xV II 0.355 ± 0.011 2.300 ± 0.0 0.849 ± 0.004 303.4 ± 17.8 248.2 ± 17.1 3.2 ± 0.6 25
xV III 0.324 ± 0.022 2.2 ± 0.0 0.855 ± 0.010 232.3 ± 17.7 293.5 ± 17.5 3.8 ± 0.8 236
xIX 0.304 ± 0.014 2.3 ± 0.0 0.870 ± 0.006 124.8 ± 12.0 71.4 ± 11.9 6.4 ± 0.7 16
xX 0.350 ± 0.015 2.3 ± 0.0 0.850 ± 0.006 226.7 ± 13.7 323.8 ± 13.5 3.6 ± 0.7 37
tev = 16 kyr, β = 0.0001
xI 0.267 ± 0.010 2.200 ± 0.0 0.880 ± 0.004 117.4 ± 11.3 351.0 ± 11.3 5.5 ± 0.5 184
xIV 0.272 ± 0.017 2.200 ± 0.0 0.878 ± 0.007 57.1 ± 16.2 51.4 ± 16.2 5.8 ± 1.0 533
tev = 16 kyr, β = 0.001
xI 0.199 ± 0.015 1.600 ± 0.100 0.873 ± 0.007 135.2 ± 13.3 339.7 ± 16.2 7.6 ± 1.2 1152
xIIb 0.193 ± 0.012 1.5 ± 0.0 0.873 ± 0.006 48.4 ± 12.0 63.6 ± 11.1 7.7 ± 1.3 565
xIV 0.204 ± 0.015 1.7 ± 0.0 0.878 ± 0.007 227.9 ± 16.5 259.2 ± 15.9 6.2 ± 1.3 580
tev = 16 kyr, β = 0.003
xI 0.203 ± 0.012 0.900 ± 0.100 0.776 ± 0.007 27.0 ± 5.1 79.5 ± 4.1 13.2 ± 0.9 150
xII 0.195 ± 0.016 0.8 ± 0.1 0.744 ± 0.012 329.1 ± 14.3 125.2 ± 8.9 11.4 ± 2.0 811
xIII 0.185 ± 0.008 0.700 ± 0.100 0.746 ± 0.006 346.8 ± 3.2 109.0 ± 3.5 11.5 ± 0.5 161
tev = 16 kyr, β = 0.005
xI 0.273 ± 0.018 1.0 ± 0.100 0.715 ± 0.004 132.4 ± 11.3 339.1 ± 59.5 7.4 ± 0.6 104
xII 0.248 ± 0.018 0.8 ± 0.100 0.673 ± 0.016 33.6 ± 8.9 73.8 ± 5.9 11.1 ± 0.9 93
xIII 0.357 ± 0.032 1.400 ± 0.100 0.745 ± 0.010 237.7 ± 16.2 274.1 ± 14.2 6.1 ± 0.8 139
xIV 0.459 ± 0.040 1.8 ± 0.1 0.746 ± 0.012 66.7 ± 11.5 127.6 ± 11.9 6.9 ± 0.5 119
tev = 16 kyr, β = 0.007
xI 0.357 ± 0.016 1.100 ± 0.100 0.672 ± 0.005 125.4 ± 7.2 7.6 ± 6.3 7.3 ± 0.3 39
xII 0.317 ± 0.044 0.800 ± 0.200 0.619 ± 0.021 39.1 ± 11.8 74.9 ± 7.9 10.7 ± 1.1 52
xIII 0.557 ± 0.017 1.800 ± 0.0 0.697 ± 0.012 293.5 ± 12.0 254.9 ± 12.1 4.3 ± 0.2 21
xIV 0.512 ± 0.038 1.700 ± 0.100 0.704 ± 0.011 246.6 ± 12.3 293.0 ± 12.0 4.9 ± 0.5 30

Notes. tev, β, and Ns: as in Table A.1; q: mean perihelion distance; a: mean semi-major axis; e: mean eccentricity; ω: mean argument of perihelion; Ω: mean longitude of ascending node; and i: mean inclination to the ecliptic. Quantities q and a are given in astronomical units and angular elements in degrees.

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