Qabs (solid lines) and Qsca (dashed lines) for CMM grains with cores of amorphous carbon (left) and cores of amorphous silicate of olivine type (middle) and pyroxene type (right) for different grain radii in μm. The inner mantle is aromatic-rich and the outer mantle aliphatic-rich amorphous carbon. At long wavelengths Qabs and Qsca increase with increasing grain size.
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