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Published online by Cambridge University Press: 03 August 2017
We made 13CO and C180 (both J = 1 — 0) maps of the 4′ × 4′ (0.2 pc × 0.2 pc) area toward TMC1-C and ρ-Oph core with the 45-m telescope of the Nobeyama radio Observatory in order to find small scale velocity fluctuation in molecular clouds based on the analysis described by Kleiner and Dickman (1987).