Table 1
Clusters used as template data set to select SFRs and other stellar clusters.
Literature name | Flag | Reference | l (deg) | b (deg) | r50 (deg) | d (pc) | log t (yr) | N |
---|---|---|---|---|---|---|---|---|
[LK2002] Cl10 | 1 | Le Duigou & Knodlseder (2002) | 79.867 | −0.908 | 0.886 | 1557 | 167 | |
65.78-2.61 | 2 | Avedisova (2002) | 66.153 | −3.123 | 1.194 | 1324 | 134 | |
Rosette | 3 | Zucker et al. (2020) | 206.438 | −1.903 | 2.025 | 1571 | 7.1 | 810 |
NGC 6530 | 4 | Dias et al. (2002) | 6.060 | −1.287 | 1.020 | 1364 | 635 | |
NGC 6531 | 5 | Dias et al. (2002) | 7.585 | −0.338 | 1.634 | 1350 | 8.6 | 804 |
UBC386 | 6 | Cantat-Gaudin & Anders (2020) | 100.562 | 8.694 | 1.147 | 1280 | 6.8 | 193 |
Ass Cyg OB9 | 7 | Sitnik (2003) | 78.753 | 1.778 | 2.293 | 1339 | 8.1 | 616 |
Serpens South molecular cloud | 8 | Fernández-López et al. (2014) | 29.364 | 2.870 | 0.976 | 920 | 123 | |
CygOB7 CO Complex | 9 | Dutra & Bica (2002) | 92.653 | 2.529 | 0.950 | 1123 | 46 | |
BRC 27 | 10 | Rebull et al. (2013) | 224.621 | −2.244 | 3.027 | 1233 | 6.9 | 1709 |
[DB2002b] G352.16+3.07 | 11 | Otrupcek et al. (2000) | −7.866 | 3.002 | 4.764 | 1169 | 7.0 | 2357 |
IC 1396 | 12 | Zucker et al. (2020) | 99.236 | 4.733 | 7.407 | 945 | 7.4 | 3140 |
[MML2017] 2399 | 13 | Miville-Deschênes et al. (2017) | 33.890 | 0.643 | 2.543 | 609 | 130 | |
Chamaeleon II | 14 | Zucker et al. (2020) | −56.363 | −14.720 | 2.452 | 200 | 41 | |
Cepheus | 15 | Zucker et al. (2020) | 108.911 | 4.359 | 9.748 | 923 | 8.2 | 11445 |
NGC 7039 | 16 | Cantat-Gaudin & Anders (2020) | 88.350 | −1.717 | 5.322 | 767 | 7.3 | 1048 |
[YDM97] CO 14 | 17 | Yonekura et al. (1997) | 104.508 | 13.950 | 3.039 | 350 | 124 | |
Serpens | 18 | Zucker et al. (2020) | 28.783 | 3.082 | 10.166 | 455 | 7.2 | 2388 |
IC 348 | 19 | Cantat-Gaudin & Anders (2020) | 160.790 | −15.812 | 11.430 | 334 | 7.4 | 2661 |
Chamaeleon I | 20 | Zucker et al. (2020) | −62.781 | −15.444 | 3.099 | 192 | 156 | |
Taurus | 21 | Zucker et al. (2020) | 172.114 | −15.302 | 4.551 | 131 | 112 | |
Ophiuchus | 22 | Zucker et al. (2020) | −8.024 | 18.781 | 12.655 | 144 | 2398 | |
Corona Australis | 23 | Zucker et al. (2020) | −0.132 | −17.592 | 3.291 | 155 | 107 | |
[DB2002b] G302.72+4.67 | 24 | Dutra & Bica (2002) | −57.143 | 4.739 | 5.854 | 112 | 235 | |
Pozzo 1 | 25 | Cantat-Gaudin & Anders (2020) | 261.858 | −8.321 | 13.343 | 398 | 8.3 | 6001 |
ASCC32 | 26 | Cantat-Gaudin & Anders (2020) | 237.327 | −9.186 | 9.878 | 818 | 8.4 | 4416 |
LacOB1 | 27 | Chen & Lee (2008) | 96.762 | −15.032 | 11.268 | 548 | 7.4 | 2367 |
RSG8 | 28 | Cantat-Gaudin & Anders (2020) | 109.331 | −1.212 | 12.055 | 468 | 7.4 | 2900 |
NGC 2451B | 29 | Cantat-Gaudin & Anders (2020) | 253.198 | −7.499 | 9.513 | 401 | 7.6 | 2826 |
NGC 2232 | 30 | Cantat-Gaudin & Anders (2020) | 215.533 | −7.983 | 13.427 | 372 | 7.2 | 1703 |
Sco OB2 UCL | 31 | de Zeeuw et al. (1999) | −29.000 | 16.813 | 15.052 | 145 | 1189 | |
IC 2602 | 32 | Cantat-Gaudin & Anders (2020) | −70.259 | −5.011 | 6.825 | 151 | 7.6 | 315 |
NGC 2516 | 33 | Cantat-Gaudin & Anders (2020) | −86.236 | −15.931 | 6.881 | 427 | 7.6 | 1156 |
Melotte 20 | 34 | Cantat-Gaudin & Anders (2020) | 147.504 | −6.461 | 8.867 | 174 | 7.7 | 414 |
Melotte 22 | 35 | Cantat-Gaudin & Anders (2020) | 166.573 | −23.406 | 5.882 | 137 | 7.9 | 296 |
NGC 2422 | 36 | Cantat-Gaudin & Anders (2020) | 230.995 | 3.061 | 6.238 | 500 | 8.0 | 347 |
Alessi 12 | 37 | Cantat-Gaudin & Anders (2020) | 67.678 | −11.723 | 3.977 | 546 | 8.1 | 127 |
NGC 3532 | 38 | Cantat-Gaudin & Anders (2020) | −72.815 | 2.279 | 4.851 | 561 | 8.6 | 88 |
IC 6451 | 39 | Cantat-Gaudin & Anders (2020) | −19.939 | −7.821 | 1.257 | 1068 | 9.2 | 86 |
NGC 6087 | 40 | Cantat-Gaudin & Anders (2020) | −32.077 | −5.426 | 2.532 | 1007 | 8.0 | 77 |
Alessi 62 | 41 | Cantat-Gaudin & Anders (2020) | 53.676 | 8.773 | 3.561 | 622 | 8.4 | 87 |
UPK 33 | 42 | Cantat-Gaudin & Anders (2020) | 27.965 | 0.108 | 3.931 | 518 | 8.4 | 111 |
NGC 1647 | 43 | Cantat-Gaudin & Anders (2020) | 180.355 | −16.861 | 2.141 | 606 | 8.6 | 272 |
NGC 6124 | 44 | Cantat-Gaudin & Anders (2020) | −19.205 | 6.078 | 5.404 | 648 | 8.3 | 1102 |
NGC 6494 | 45 | Cantat-Gaudin & Anders (2020) | 9.714 | 2.980 | 5.537 | 755 | 8.6 | 680 |
IC 4725 | 46 | Cantat-Gaudin & Anders (2020) | 14.022 | −4.595 | 4.807 | 669 | 8.1 | 788 |
Alessi 44 | 47 | Cantat-Gaudin & Anders (2020) | 37.075 | −11.510 | 7.285 | 587 | 8.2 | 637 |
Stock2 | 48 | Cantat-Gaudin & Anders (2020) | 133.371 | −1.160 | 8.292 | 384 | 8.6 | 727 |
NGC 2168 | 49 | Cantat-Gaudin & Anders (2020) | 186.647 | 2.327 | 2.616 | 928 | 8.2 | 118 |
DSHJ2320.1+5821A | 50 | Kronberger et al. (2006) | 111.248 | −2.785 | 2.394 | 1131 | 243 | |
UPK 143 | 51 | Cantat-Gaudin & Anders (2020) | 91.810 | 0.514 | 1.752 | 934 | 8.4 | 262 |
Collinder421 | 52 | Cantat-Gaudin & Anders (2020) | 79.429 | 2.527 | 1.061 | 1265 | 8.4 | 154 |
Notes. Flag is the value assigned to each cluster to characterise a given observed CAMD shape. r50 is the radius in which half of the identified members are concentrated, d is the distance obtained by inverting the median value of the member parallaxes and N is the number of members. Flag = [1, 28] are assigned to clusters with ages t ≲ 10 Myr, Flag = [29, 36] are assigned to clusters with ages 10 ≲ t/ Myr ≲ 100, Flag = [37,52] are assigned to clusters with ages t ≳ 100 Myr.
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