Constraints on Cosmic Ray propagation from Radio Continuum data of NGC 2146

We present high-sensitivity multi-frequency radio continuum observations of the starburst galaxy NGC~2146. We have fitted these data with a three-dimensional diffusion model. The model can describe the radio emission from the inner disk of NGC~2146 well, indicating that diffusion is the dominant mode of propagation in this region. Our results are indicating that NGC~2146 has recently undergone a starburst, the star forming activity being located in a central bar. The spatial variation of the radio emission and of the spectral index yield tight constraints on the diffusion coefficient $D_0$ and the energy dependence of the diffusion. Away from the central bar of the galaxy the radio emission becomes filamentary and the diffusion model was found to be a poor fit to the data in these regions; we attribute this to different transport processes being important in the halo of the galaxy.