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Table 2

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

Fil. tevol; D.B. D lim q a e ω Ω i N sel.
F1 20 kyr 0.19 0.819 ± 0.028 17.737 ± 2.219 0.953 ± 0.006 127.9 ± 2.4 39.7 ± 3.7 66.1 ± 2.1 176
F1 30 kyr 0.19 0.805 ± 0.031 21.329 ± 3.422 0.961 ± 0.006 125.7 ± 3.0 37.5 ± 3.0 65.3 ± 2.4 290
F1 40 kyr 0.21 0.790 ± 0.035 23.776 ± 5.354 0.965 ± 0.006 123.4 ± 3.8 37.7 ± 4.0 66.0 ± 2.8 289
F1 50 kyr 0.28 0.779 ± 0.045 24.739 ± 6.646 0.967 ± 0.007 122.4 ± 5.1 37.8 ± 5.0 66.2 ± 3.3 406
F1 V 0.18 0.841 ± 0.029 9.474 ± 9.261 0.894 ± 0.070 130.7 ± 4.8 37.3 ± 3.4 72.6 ± 4.7 22
F1 R 0.20 0.768 ± 0.041 23.569 ± 37.297 0.922 ± 0.051 120.5 ± 5.2 47.8 ± 2.8 67.2 ± 5.8 14
F2 40 kyr 0.17 0.291 ± 0.044 172.693 ± 56.760 0.998 ± 0.000 67.4 ± 6.3 152.5 ± 8.0 30.6 ± 1.7 35
F2 50 kyr 0.14 0.253 ± 0.032 75.925 ± 23.856 0.996 ± 0.001 60.9 ± 4.4 157.8 ± 5.5 30.6 ± 1.7 89
(F2 V 0.25 0.115 ± 0.051 8.059 ± 9.500 0.969 ± 0.036 35.6 ± 10.1 173.0 ± 10.3 24.0 ± 3.9) 13
(F2 R 0.18 0.385 ± 0.047 2.259 ± 0.826 0.810 ± 0.067 66.8 ± 6.8 148.3 ± 6.5 33.7 ± 3.3) 10
(F2 R 0.17 0.222 ± 0.051 1.942 ± 0.957 0.865 ± 0.060 46.2 ± 7.2 178.2 ± 6.8 29.9 ± 3.6) 13
F3 10 kyr 0.14 0.213 ± 0.020 28.245 ± 6.748 0.992 ± 0.002 124.5 ± 3.6 83.9 ± 5.0 34.2 ± 2.0 1626
F3 20 kyr 0.13 0.206 ± 0.024 36.197 ± 8.489 0.994 ± 0.002 126.0 ± 3.2 79.7 ± 4.7 35.5 ± 2.1 898
F3 30 kyr 0.16 0.204 ± 0.028 37.793 ± 7.138 0.994 ± 0.002 126.4 ± 4.0 76.4 ± 5.2 36.2 ± 2.6 533
F3 40 kyr 0.21 0.197 ± 0.030 35.578 ± 7.143 0.994 ± 0.001 127.4 ± 4.5 74.5 ± 5.7 37.9 ± 3.4 531
F3 50 kyr 0.25 0.210 ± 0.031 34.549 ± 6.890 0.994 ± 0.001 125.2 ± 4.6 77.3 ± 6.0 34.9 ± 3.8 479
(F3 F 0.10 0.189 ± 0.017 53.035 ± 67.069 0.990 ± 0.012 128.7 ± 2.1 80.1 ± 2.5 35.9 ± 2.1 14)
F3 F 0.22 0.168 ± 0.040 100.343 ± 210.941 0.990 ± 0.023 132.1 ± 6.1 76.4 ± 6.4 31.7 ± 5.7 23
(F3 V 0.09 0.187 ± 0.018 15.571 ± 20.716 0.983 ± 0.014 129.3 ± 2.7 78.7 ± 3.1 35.3 ± 1.9 388)
F3 V 0.22 0.153 ± 0.045 14.792 ± 23.138 0.984 ± 0.021 135.1 ± 7.5 73.1 ± 8.0 29.6 ± 6.0 1268
(F3 R 0.11 0.183 ± 0.016 8.749 ± 4.346 0.969 ± 0.033 131.1 ± 2.4 77.3 ± 3.0 35.4 ± 2.7 11)
F3 R 0.16 0.146 ± 0.045 31.823 ± 117.770 0.976 ± 0.036 136.6 ± 6.8 72.2 ± 6.5 23.8 ± 3.5 62
F4 40 kyr 0.07 0.821 ± 0.037 12.681 ± 1.000 0.935 ± 0.008 53.9 ± 2.9 15.3 ± 5.0 71.8 ± 0.7 2
F4 50 kyr 0.14 0.753 ± 0.017 14.439 ± 0.802 0.948 ± 0.003 56.1 ± 1.4 7.2 ± 6.2 71.6 ± 0.7 4
(F4 V 0.23 0.746 ± 0.034 20.716 ± 35.115 0.893 ± 0.079 62.1 ± 4.1 22.7 ± 3.4 70.5 ± 6.5 7)

Notes. tevol and Dlim – as in Table. 1; D.B. – database from which the observed counterpart of the filament is selected (F – photographic; V – video-meteor; R – radio-meteor database); q – perihelion distance; a – semi-major axis; e – eccentricity; ω – argument of perihelion; Ω – longitude of ascending node; i – inclination to the ecliptic; and Nsel. – the number of particles or real meteors selected from the modeled set (of 10000 particles) or from given database. Quantities q and a are given in astronomical units and angular elements in degrees.

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