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Fig. 1

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JHKs true colour images of the three clusters. Stars marked by circles were observed using near infrared spectrographs. In green are the stars observed using SofI at NTT and in red are the stars observed with MMIRS at the Clay telescope. The stars marked with a yellow circle in RCW 79 were already observed by Martins et al. (2010) and, hence, were not re-observed by us.

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