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Booth","submitted_at":"2012-02-20T19:49:37Z","abstract_excerpt":"We have mapped faint 1667 OH line emission (TA \\approx 20 - 40 mK in our \\approx 30' beam) along many lines of sight in the Galaxy covering an area of \\approx 4\\circ \\times 4\\circ in the general direction of l \\approx 108\\circ, b \\approx 5\\circ. The OH emission is widespread, similar in extent to the local HI (r </= 2 kpc) both in space and in velocity. The OH profile amplitudes show a good general correlation with those of HI in spectral channels of \\approx 1 km/s; this relation is described by TA(OH) \\approx 1.50 \\times 10^{-4} TB(HI) for values of TB(HI) </\\approx 60 - 70 K. 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