The nature of OH 0739 – 14

Abstract
We show that the OH source OH0739 –14 (= OH 231.84 +4.22) comprises a late-type star engulfed within an extensive reflection nebula. The nebula probably was generated by prolonged mass loss. The reddening law within the nebula appears to be abnormal. We suggest that such objects may be rather commonplace in the Galaxy's halo.

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