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Fig. 3


VLA 3.6 cm radio continuum image of K 3-35 overplotted by H2-Kc (left) and [S iv] (right) contours. The spatial scale is indicated in the left panel. The bright point source west of the central core in the continuum-subtracted H2 contours at PA ~ 260° corresponds to a field star not properly subtracted (see text). The contours overplotted are in logarithmic scale to enhance the morphological features detected.

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