Fig. 1
1.2 mm dust continuum MAMBO mosaic of the Aquila rift complex, smoothed to an effective angular resolution of 13. Due to the high dynamic range of fluxes in the map, and to enhance visibility of the structure of emission in the whole area mapped, the color scale chosen here has a maximum of 400 mJy/beam. The highest flux density of order ~1400 mJy/beam is found in the center of the Serpens South protocluster (see the blow-up in Fig. 2). In this smoothed map, the mean rms noise level is ~13 mJy/13-beam.
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