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Fig. 1


Large-scale image of the 4.5 μm emission towards the star-forming region G35.20–0.74 N overlaid with a contour map of the 350 GHz continuum emission obtained with ALMA. The IR image has been obtained by applying HiRes deconvolution (Velusamy et al. 2008) to the Spitzer/IRAC data. The sub-mm map has been corrected for primary beam attenuation. The contours range from 9 to 203 mJy/beam in steps of 10.8 mJy/beam. The dashed circle denotes the primary beam of the ALMA 12-m antennas. The ellipse in the bottom right is the ALMA synthesized beam.

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