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Table A.1.
Observation of the high-mass tail of the stellar initial mass function of different stellar cluster and their stellar mass. These values are plotted in figure 9
| name | α | M*[M⊙] | year | Reference |
|---|---|---|---|---|
| Taurus | 1.815 ± 0.324 | 87.0 | 2014 | |
| IC 348 | 1.267 ± 0.313 | 82.22 | 2014 | |
| NGC 6611 | 1.954 ± 0.221 | 250.3 | 2014 | |
| NGC 2264 | 1.717 ± 0.14 | 574.8 | 2014 | Dib (2014) |
| ONC | 1.236 ± 0.007 | 693.5 | 2014 | |
| ρ Oph | 0.875 ± 0.293 | 96.49 | 2014 | |
| Cha I | 1.139 ± 0.367 | 30.42 | 2014 | |
| NGC 3603 | 0.85 ± 0.1 | 9700.0 | 2008 | Harayama et al. (2008) |
| 30 Doradus | 0.95 ± 0.26 | 4×104 | 2018 | Schneider et al. (2018), Andersen et al. (2009) |
| Arches | 0.8 ± 0.06 | 2×104 | 2018 | Hosek et al. (2019) |
| Cyg OB2 | 1.39 ± 0.19 | 1.65×104 | 2015 | Wright et al. (2015) |
| h Per | 1.3 ± 0.2 | 3700 | 2002 | Slesnick et al. (2002) |
| χ Per | 1.36 ± 0.20 | 2800 | 2002 | |
| M35 | 1.29 ± 0.27 | 1600 | 2003 | Kalirai et al. (2003) |
| M50 | 1.94 ± 0.15 | 1100 | 2003 | |
| NGC 346 | 1.43± 0.18 | 3×104 | 2007 | Sabbi et al. (2008) |
| Ple | 1.7 ± 0.2 | 740 | 2004 | Moraux et al. (2004) |
| Quint | 0.68 ± 0.13 | 6000 | 2012 | Hußmann et al. (2012) |
| Sh 2-209 | 1 ± 0.2 | 1000 | 2022 | Yasui et al. (2023) |
| Tr 14 | 1.3 ± 0.1 | 8847 | 2012 | Hur et al. (2012), Ascenso et al. (2007) |
| Wes 1 | 0.8 ± 0.1 | 7.3×104 | 2012 | Lim et al. (2013) |
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