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Table 1.

Stellar groups recovered by SNN.

SNN Parent Size Stability Group name Blaauw Reference
1 681 3408 81.75 (0.84) 2.29 (1.01) 2.85 (0.09) 1.45 (0.23) −0.29 (0.33) Briceno 1 Ia Briceño et al. (2007)
2 149 3241 87.83 (1.01) −7.92 (1.48) 3.34 (0.12) 0.19 (0.22) −0.58 (0.21) Orion Y Kounkel et al. (2018)
3 432 2852 83.69 (1.21) −1.62 (0.72) 2.77 (0.08) 1.64 (0.33) −1.25 (0.23) OBP-near Ib This work
4 630 2743 83.92 (0.99) 9.77 (0.83) 2.47 (0.1) 1.26 (0.41) −2.19 (0.25) λ Ori Murdin & Penston (1977)
5 871 2240 83.83 (0.38) −6.02 (0.64) 2.59 (0.09) 1.2 (0.21) 0.45 (0.24) NGC 1980 Ic Alves & Bouy (2012)
6 202 1918 83.21 (0.55) −1.55 (0.5) 2.36 (0.08) 0.04 (0.18) −0.18 (0.21) OBP-d Ib Kubiak et al. (2017)
7 141 1403 81.98 (0.6) 1.64 (0.58) 2.71 (0.08) −0.58 (0.21) 0.75 (0.21) ASCC20 Ia Kharchenko et al. (2013)
8 146 978 78.36 (1.01) −2.43 (0.79) 2.61 (0.08) 1.39 (0.19) −0.65 (0.18) L1616 This work
9 123 947 84.31 (0.52) −0.68 (0.52) 2.57 (0.08) −1.11 (0.19) −0.72 (0.18) OBP-b Ib Kubiak et al. (2017)
10 78 739 86.12 (0.89) 7.29 (1.04) 2.2 (0.1) −3.3 (0.19) −1.72 (0.2) λ Ori South This work
11 80 647 77.99 (1.17) −8.18 (2.19) 3.54 (0.17) 1.75 (0.24) −2.99 (0.22) Rigel This work
12 151 425 85.7 (0.5) −8.11 (0.67) 2.29 (0.08) 0.09 (0.23) −0.28 (0.22) L1641S Id Strom et al. (1993)
13 3 381 358 84.16 (0.89) −1.53 (0.76) 2.77 (0.09) 1.78 (0.23) −1.26 (0.24) This work
14 106 158 83.38 (0.74) 3.97 (0.93) 2.35 (0.08) −0.94 (0.25) 0.6 (0.19) ome Ori Ia This work
15 64 126 76.35 (1.03) 12.41 (1.2) 3.2 (0.15) 1.8 (0.29) −3.55 (0.2) L1562 This work
16 77 110 81.58 (0.77) 0.45 (0.68) 2.37 (0.08) 0.21 (0.24) 1.43 (0.18) OBP-West This work
17 115 84 85.58 (0.66) −9.32 (0.86) 2.18 (0.08) 0.53 (0.22) −1.19 (0.24) L1647 This work
18 3 367 49 84.3 (0.8) −1.63 (0.78) 2.76 (0.1) 1.8 (0.21) −1.3 (0.24) This work
19 105 39 83.83 (0.53) −1.64 (0.81) 2.31 (0.07) −1.38 (0.21) 0.93 (0.19) OBP-far Ib This work
20 135 37 80.06 (1.24) −4.1 (1.28) 3.09 (0.09) 0.87 (0.18) −0.43 (0.14) Orion X Bouy & Alves (2015)
21 71 35 81.03 (0.39) −4.29 (0.41) 2.61 (0.07) 1.93 (0.21) −1.0 (0.18) L1634 This work
22 53 27 88.9 (0.72) 0.45 (1.08) 2.38 (0.11) −2.12 (0.17) −2.1 (0.2) Orion B East This work
23 66 26 80.09 (2.25) −9.94 (1.69) 3.53 (0.16) −0.17 (0.19) −1.26 (0.19) Orion Y extension This work
24 64 22 87.39 (0.95) −5.06 (0.83) 2.2 (0.09) −2.49 (0.22) 0.26 (0.2) Orion A East This work
25 4 150 12 84.03 (0.51) 9.73 (0.5) 2.49 (0.08) 0.96 (0.22) −2.14 (0.18) This work

Notes. Each row corresponds to one distinct stellar group identified by either algorithm. The names in bold highlight the newly discovered groups. The columns from left to right show for each group: (1) the SNN group index; (2) the SNN group index of the immediate group that contains, or partially contains it; (3) the number of stars it contains; (4) the number of times it appears out of 7000 SNN runs; (5) the average RA; (6) the average Dec; (7) the average parallax; (8) the average PMRA; (9) the average PMDec; (10) identifier from previous works if already known and from this work in bold if newly discovered; (11) the Blaauw structure to which it belongs; (12) reference for the identifier in (10). The numbers in parentheses from Cols. (5) to (9) are the standard deviations of the quantities shown.

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