2009A&A...507L..25C

L1157-mm is a low-mass protostar driving an outflow which is considered the proto-type of the so-called chemically active outflows. In particular, the blue-shifted lobe B1 stands out for its rich mm-wave spectrum. Our aim is to infer the physical conditions of the molecular gas within L1157-B1. We carried out CH₃CN(8_K-7_K) observations at 2mm with the IRAM Plateau de Bure Interferometer to map L1157-B1. The CH₃CN image shows a clumpy structure superimposed to the classical B1 arch-like shape, displaying a unique continuous structure tracing the propagation of a large bow shock. The CH₃CN spatial distribution well agrees with that of CH₃OH, one of the most abundant species evaporated from dust grain mantles. Thanks to the present CH₃CN observations at unprecedented spatial resolution, we determine for the first time the temperature distribution of the B1 bow shock. We obtain values between 57 and 132K, with the highest temperature at the shock apex, thus confirming the association of CH₃CN with gas affected by the passage of a shock wave. The N_CH3_CN column densities are ≃8-40x10¹²cm^–2, depending on the position, leading to CH₃CN/CH₃OH abundance ratios ≃0.2-1.3x10^–3, i.e. values on average smaller than those found in hot-corinos. This suggests that a significant amount of CH₃CN is formed in the gas phase: in the shocked L1157-B1 regions the CH₃CN abundance may not have reached its maximum yet.