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Table 1.

References for the chemical properties of globular and open clusters used in the comparison with model predictions.

Cluster MTO Age Ref. Mass & Age Ref. [C/N] Symbols
Tr 20 1.9 1.4 Carraro et al. (2010); Donati et al. (2014) GES Black plus sign
NGC 104 0.89 12 Charbonnel & Chantereau (2016) GES Dark cyan circle
according to VandenBerg et al. (2013) and Parada et al. (2016)
NGC 1851 0.87 11 Charbonnel & Chantereau (2016) GES Magenta square
according to VandenBerg et al. (2013)
NGC 5927 0.94 11 Charbonnel & Chantereau (2016) GES Blue diamond
according to VandenBerg et al. (2013)
NGC 6705 3.30 0.3 Santos et al. (2005) GES Yellow square
Cantat-Gaudin et al. (2014)
NGC 2243 1.19 4.5 WEBDA database GES Red square
Br 81 2.06 1.0 Sagar & Griffiths (1998) GES Blue open diamond
NGC 6005 2.05 1.2 Piatti et al. (1998) GES Black down triangle
NGC 6802 1.90 0.9 Tang et al. (2017) GES Purple circle
Tr 23 2.05 0.8 Overbeek et al. (2017) GES Green square
Br 31 1.52 2.9 Cignoni et al. (2011) GES Yellow open square
Br 36 1.39 7 Donati et al. (2012) GES Magenta plus sign
Melotte 71 3.65 0.2 WEBDA database GES Pink open circle
NGC 6067 4.75 0.1 WEBDA database GES Magenta circle
according to Alonso-Santiago et al. (2017)
NGC 6253 1.32 3-5 WEBDA database GES Purple plus sign
M67 1.6 2.6 WEBDA database GES Green circle
NGC 6259 3.73 0.2 WEBDA database GES Dark blue circle
Dias et al. (2002)
Rup 134 2.18 1.0 Carraro et al. (2006) GES Red circle

NGC 2324 2.7 0.44 Tautvaišienė et al. (2016) Red cross
NGC 3960 2.2 0.9 Tautvaišienė et al. (2016) Blue plus sign
NGC 6253 1.4 0.6 Mikolaitis et al. (2012) Black open circle
NGC 2477 2.3 0.82 Tautvaišienė et al. (2016) Magenta up triangle
Melotte 66 1.2 4 Drazdauskas et al. (2016) Black cross
Collinder 261 1.1 6.0 Mikolaitis et al. (2012) Yellow circle
Drazdauskas et al. (2016)
NGC 6134 2.34 0.7 Mikolaitis et al. (2010) Blue open square
NGC 2506 1.69 1.7 Mikolaitis et al. (2011a) Green up triangle
IC 4651 1.69 1.7 Mikolaitis et al. (2011b) Red down triangle

Notes. For GES clusters, the approximate turn-off masses were evaluated using the theoretical PARSEC isochrones (Bressan et al. 2012) with the corresponding ages and metallicities. For globular clusters see the text; for clusters already published, we use the turn-off mass and age indicated in the corresponding article.

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