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Fig. 1

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1.2 mm dust continuum emission (contours, plotted in steps of 3σ) overplotted on a NIR K image of CB 17 (Launhardt et al. 2010). The arrows represent the red- and blue-shifted components of the outflow detected by Chen et al. (2012). The grey circle in the bottom left corner represents the angular resolution of the 1.2 mm dust continuum image. The coordinate offsets are given w.r.t. to the position of IRS (αJ2000=04h04m3376, δJ2000=+56°56165, Chen et al. 2012).

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