2004A&A...416..631B

We present high angular resolution interferometric observations of the dust continuum at 2.7 and 1.3mm, and of the HC₃N (J=12-11) and C¹⁸O (J=2-1) emission around L1157-mm, a Class 0 object that drives a spectacular molecular outflow. The millimeter dust emission is clearly resolved into two components, a flattened compact source of ∼450x250AU at 1.3mm, and mass ∼0.1M_☉, plus an extended envelope of ∼3000AU at 1.3mm, and mass ∼1.1M_☉. The millimeter spectral index varies throughout the region, with the lower value found toward the compact protostar, possibly indicating grain growth in the denser regions. A strong interaction between the molecular outflow and the close protostellar environment is taking place and affects the structure of the innermost parts of the envelope. This is shown by the spatial coincidence between the molecular outflow and the dust (1.3mm continuum) and HC₃N emission: both tracers show structures associated to the edges of the outflow lobes. Basically, the global picture sketched for the Class 0 object L1157-mm by Gueth et al. (1997A&A...323..943G) is supported. We find possible evidence of infall, but we do not detect any velocity gradient indicative of a rotating circumstellar disk.