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Near-infrared linear imaging polarimetry of the young stellar objects R CrA and T CrA in the J, H and Kn bands, and circular imaging polarimetry in the H band, is presented. The data are modelled with the Clark and McCall scattering model. The R CrA and T CrA system is shown to be a particularly complex scattering environment. In the case of R CrA there is evidence that the wavelength dependence o...

Polarization models of young stellar objects -- II. Linear and circular polarimetry of R Coronae Australis