Fig. 2.
Left panels: SMA 230 GHz thermal dust continuum emission towards G10.99−0.08 (top panel) and G28.33+0.07 (bottom panel). The levels start at 2σ, 3σ, in steps of 2σ. Right panels: SMA CO 2-1 integrated intensity emission at high velocities as contours overlaid on SMA dust continuum observations towards G10.99−0.08 (top panel) and G28.33+0.07 (bottom panel). The contours start at 6σ, in steps of 2σ. The circle shows the SMA FOV at 230 GHz. The ellipse in the lower left corner represents the SMA synthesized beam size. The magenta star in the top left panel for G10.99−0.08 corresponds to a Herschel identified low-mass protostar outside the SMA FOV by Henning et al. (2010).
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