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Table 2
Star formation efficiency for each cluster.
Name | Gas mass | SFEB | SFEF |
M⊙ | % | % | |
|
|||
NGC 2244 | 1518 | 36.1 | 30.2 |
NGC 2237 | 316 | 28.1 | 22.6 |
PL01 | 1201 | 13.7 | 5.2 |
PL02 | 469 | 17.0 | 7.6 |
PL03 | 2075 | 16.4 | 6.6 |
PL04 | 4834 | 19.4 | 8.4 |
PL05 | 2049 | 23.8 | 10.2 |
REFL08 | 3133 | 13.8 | 3.2 |
PL06 | 2893 | 11.3 | 3.9 |
PL07 | 901 | 12.7 | 4.8 |
REFL09 | 2163 | 10.3 | 3.4 |
CMFT10 | 472 | 15.3 | 8.7 |
CMFT11 | 233 | 19.5 | 12.3 |
Notes. Two SFE values are proposed to account for the uncertainty on the cluster locations with respect to the molecular cloud (the superscript B and F letters refer to the back and front side location as in Table 1).
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