Thermal structure of the simulated core. Left: Radial profiles for the dust temperature along 8 different radial cuts on the x-y, z-x, and z-y planes. The profiles for the 1D hydrodynamical model from Keto & Caselli (2010) is indicated by the black dotted line. Right: Greyscale images shows the continuum emission of the core at 1.1 mm, while contours indicate 15%, 30%, 45%, 60%, and 75 % of the peak intensity. The dotted colored lines indicate the direction along which the radial profiles in the other panel were extracted.