Shear, writhe, and filaments: Turbulence in the high-latitude molecular cloud MBM 40

Open Access

Fig. 7

Shear flow in the western ridge of MBM 40. The pseudocolor image is H I. ¹²CO peak velocities are plotted in blue and CH in dotted white. Stars indicate the mean ¹³CO peak velocity observed with Onsala telescope in MAP1, MAP2 and MAP4. ¹²CO missing points below 0.2 pc shows too low S/N.

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