Fig. 1
Left: MIPS 24 μm image of the arcminute-scale bipolar nebula and its central star MWC 349A (a bright source in the waist of the nebula; note that a white dot at the centre of this source is due to saturation effect). Middle and right: MIPS 70 μm and VLA 17 cm images of the same field. The 47′′FWHM restoring beam is represented in the bottom right corner of the radio image.
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