Fig. 11
Velocity distribution of HI emission towards VRO 42.05.01 at the range of velocities that corresponds to the close molecular cloud. The data cube was taken from the CGPS. Overlaid are the radio contours at 1420 MHz in units of brightness temperature at 2.5, 3.7, 4.8, and 6 K. The wedges in the upper left corner of each plot correspond to the velocity of each slice. The brightness temperature TB colour scale is the same for all plots.
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