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A 2005 Chandra X-ray observation combined with multi-epoch VISTA near-infrared photometry provides a catalog of 2148 probable stellar members in the young cluster NGC 6231. This catalog, which is 70% larger than previous censuses, includes low-mass stars and B stars with newly identified X-ray counterparts. The work estimates a total population of 5700-7500 members down to 0.08 solar masses within the Chandra field.
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