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Table 1

Age estimates, reddening, distance to the Sun, and GES and Gaia membership studies from the literature for the 16 star forming regions and young clusters in our sample.

Cluster name Age (Myr) E(B – V)(a) (dex) Distance (kpc) References Ages References Distance GES and Gaia membership studies
NGC 6530 1-2 0.44 ± 0.10 1.33 3, 4, 18, 19, 20, 33 18, 19, 20, 21 2, 3, 16, 18, 19, 22
ρ Oph 1-3 0.76 ± 0.13 0.13 ± 0.01 1, 2, 3, 4, 5, 33, 61 1, 2, 6 1, 2, 3, 6
Trumpler 14 1-3 0.61 ± 0.10 2.90 3, 4, 13, 33 13, 14 2, 3, 15, 17
Cha I 2 0.18 ± 0.08 0.16 ± 0.02 3, 4, 7, 8, 9, 33 7, 8, 10, 11 2, 3, 7, 8, 10, 11(b), 12
NGC 2244 4 0.49 ± 0.09 1.59 3, 23, 24, 33 21, 23, 24, 25 3, 15, 24, 26
NGC 2264 4 0.05 ± 0.05 0.76 2, 3, 4, 27, 28, 29, 30, 33 2, 15, 25, 28, 29 2, 3, 15, 31, 32
λ Ori 6 0.09 ± 0.04 0.41 3, 43 34 3, 15
Col 197 13 0.64 ± 0.07 0.80-0.90 3, 5, 13, 35, 36, 37 13, 25, 35, 36, 37 3, 15
γ Vel 10-20 0.04 ± 0.03 0.35-0.40 2, 3, 8, 10, 38, 39, 40, 41, 42 8, 10, 38, 40, 41, 42 2, 3, 8, 10, 38, 39, 40, 41, 42, 44, 45, 46
NGC 2232 18-32 0.04 ± 0.03 0.32 3, 5, 43, 47, 48, 64 13, 25, 48 3, 15, 43, 48
NGC 2547 20-45 0.06 ± 0.03 0.36 ± 0.02 2, 3, 5, 8, 32, 41, 42, 48, 49, 50, 51, 63, 64 2, 8, 41, 42, 48 2, 3, 8, 15, 32, 42, 48, 49, 52
IC 2391 36 ± 2 (c) 0.03 ± 0.01 0.16 ± 0.01 3, 48, 51, 53, 64 2, 48, 54, 55, 56 2, 3, 15, 49, 52, 62
IC 2602 35 ± 1 (c) 0.04 ± 0.02 0.15 ± 0.01 3, 5, 48, 51, 64 2, 48, 56 2, 3, 15, 49, 52, 62
IC 4665 38 ± 3 (c) 0.15 ± 0.02 0.36 ± 0.01 3, 5, 48, 51, 64 2, 48, 57, 58 2, 3, 15, 48, 49, 52, 62
NGC 2451 B 39 ± 1 (c) 0.10 ± 0.03 0.36 3, 42, 48, 49, 51, 59, 60 42, 48, 59 2, 3, 15, 42, 48, 49
NGC 2451 A 44 ± 2 (c) 0.02 ± 0.02 0.19 3, 42, 48, 49, 51, 59, 60 42, 48, 59 2, 3, 15, 42, 48, 49

Notes. (a)References for the E(B–V) reddening adopted from Jackson et al. (2022) for all clusters. (b)GES studies that reference the clusters and/or study them without taking membership analysis primarily into account. (c)Updated cluster ages using Gaia data, as listed by Bossini et al. (2019).

References. For the cluster ages, reddening and distances shown here we chose the most recent or most robust estimates for each cluster, but several other studies are further cited here, and age estimates are additionally briefly discussed in the individual notes of Appendix A: (1) Rigliaco et al. (2016); (2) Spina et al. (2017); (3) Jackson et al. (2022); (4) Randich et al. (2020); (5) Romano et al. (2021); (6) Cánovas et al. (2019); (7) Spina et al. (2014a); (8) Sacco et al. (2015); (9) López Martí et al. (2013); (10) Frasca et al. (2015); (11) Roccatagliata et al. (2018); (12) Galli et al. (2021); (13) Sampedro et al. (2017); (14) Mel'nik & Dambis (2017); (15) Cantat-Gaudin et al. (2018); (16) Castro-Ginard et al. (2020); (17) Damiani et al. (2017); (18) Wright et al. (2019); (19) Damiani et al. (2019); (20) Prisinzano et al. (2005); (21) Kuhn et al. (2019); (22) Prisinzano et al. (2019); (23) Mužić et al. (2019); (24) Michalska (2019); (25) Kharchenko et al. (2005); (26) Carrera et al. (2019); (27) Arancibia-Silva et al. (2020); (28) Bonito et al. (2020); (29) Gillen et al. (2020); (30) Venuti et al. (2019); (31) Maíz Apellániz (2019); (32) Jackson et al. (2016); (33) Randich et al. (2022); (34) Dib et al. (2018); (35) Dias et al. (2019); (36) Bonatto & Bica (2010); (37) Vande Putte et al. (2010); (38) Jeffries et al. (2014); (39) Spina et al. (2014b); (40) Franciosini et al. (2018); (41) Beccari et al. (2018); (42) Franciosini et al. (2022b); (43) Binks et al. (2022); (44) Damiani et al. (2014); (45) Prisinzano et al. (2016); (46) Cantat-Gaudin et al. (2019); (47) Liu & Pang (2019); (48) Pang et al. (2021); (49) Randich et al. (2018); (50) Sestito & Randich (2005); (51) Bossini et al. (2019); (52) Bravi et al. (2018); (53) Dumont et al. (2021b); (54) Platais et al. (2007); (55) De Silva et al. (2013); (56) Smiljanic et al. (2011); (57) Martín & Montes (1997); (58) Jeffries et al. (2009); (59) Silaj & Landstreet (2014); (60) Netopil & Paunzen (2013); (61) Kiman et al. (2021); (62) Gómez Garrido (2015); (63) Oliveira et al. (2003), (64) Jeffries et al. (2023).

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