Properties and rotation of molecular clouds in M 33

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Fig. 1

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Left: CO(2–1) integrated intensity map of M 33 with the cloud contours superposed in red and a zoom on cloud #4 showing (top right) the velocities as measured using Eq. (1), middle right: the fit to the velocities using Eq. (2), and to the bottom right the velocity residual, all in km s ⁻¹.

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