Fig. 9
The ~1.5° × 1.5° extinction map produced by Dobashi et al. (2005) of the region containing BHR 111. The contours are drawn at 2, 2.1, 2.2, 2.3, and 2.4 mag levels. The fields used to select stars to determine distance are identified and labelled. The stars classified as dwarfs and used to determine distance to the cloud are identified using open circles.
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