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Turbulence in TMC1-C and ρ-Oph core
Published online by Cambridge University Press: 03 August 2017
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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).
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- Copyright © Kluwer 1991
References
Rieke, G. H., Ashok, N. M., and Boyle, R. P.
1989, Ap. J. (Letters), 339, L71
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