Fig. 14
The 1.5° × 1.5° extinction map produced by Dobashi et al. (2005) of the region containing L673-7. The contours are drawn at the 4.0 and 5.0 mag levels. The fields used to select stars to determine distances are identified and labelled. The stars classified as dwarfs using the near-IR photometry in each field are shown using filled circles. Each field covers an area of 0.5° × 0.5°.
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