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(10 Sep 2012) Key: citeulike:11223400
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Evidence is presented indicating that the young star cluster Westerlund~2 lies $d_odot∼3.0$ kpc in the direction of Carina. The distance is tied partly to new $UBVRI_c$ photometry and revised spectral classifications for cluster stars, which imply that dust in the direction of Carina is characterized by an anomalous extinction law ($R_V∼3.8$). That result was determined from a multi-faceted approach relying on the variable-extinction and color excess methods.
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