A Chandra X-ray study of the young star cluster NGC 6231: low-mass population and initial mass function

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Fig. 28

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Plot of X-ray luminosity L_X vs. stellar mass. Symbols as in Fig. 4. The dotted horizontal line is our completeness limit. The narrow gap at ~1.4 M_⊙ is an artifact corresponding to the transition between the BHAC and Siess et al. (2000) isochrone sets used.

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